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1,803.02267
An overview of $\Lambda_c$ decays
The decays of the ground-state charmed baryon $\Lambda_c$ are now close to being completely mapped out. In this paper we discuss some remaining open questions, whose answers can help shed light on weak processes contributing to those decays, on calculations of such quantities as transition form factors in lattice QCD, and on missing decay modes such as $\Lambda_c \to \Lambda^* \ell^+ \nu_\ell$, where $\Lambda^*$ is an excited resonance. The discussion is in part a counterpart to a previous analysis of inclusive $D_s$ decays.
hep-ph hep-ex
the decays of the groundstate charmed baryon lambda_c are now close to being completely mapped out in this paper we discuss some remaining open questions whose answers can help shed light on weak processes contributing to those decays on calculations of such quantities as transition form factors in lattice qcd and on missing decay modes such as lambda_c to lambda ell nu_ell where lambda is an excited resonance the discussion is in part a counterpart to a previous analysis of inclusive d_s decays
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1,803.02268
Potential Energy Between Static Quarks Is Time Dependent in The Classical Yang-Mills Theory
Lattice QCD predicts that the potential energy between static quarks is independent of time. However, in this paper we show that the gauge invariant color singlet potential energy between static quarks in the classical Yang-Mills theory depends on time even if the quarks are at rest. This is a consequence of the time dependent fundamental color charge $q^a(t)$ of the quark in the classical Yang-Mills theory. We find that the gauge invariant color singlet time dependent potential energy between static quarks does not violate the conservation of energy in the Yang-Mills theory.
hep-ph hep-lat nucl-th
lattice qcd predicts that the potential energy between static quarks is independent of time however in this paper we show that the gauge invariant color singlet potential energy between static quarks in the classical yangmills theory depends on time even if the quarks are at rest this is a consequence of the time dependent fundamental color charge qat of the quark in the classical yangmills theory we find that the gauge invariant color singlet time dependent potential energy between static quarks does not violate the conservation of energy in the yangmills theory
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1,803.02269
Personalized Exposure Control Using Adaptive Metering and Reinforcement Learning
We propose a reinforcement learning approach for real-time exposure control of a mobile camera that is personalizable. Our approach is based on Markov Decision Process (MDP). In the camera viewfinder or live preview mode, given the current frame, our system predicts the change in exposure so as to optimize the trade-off among image quality, fast convergence, and minimal temporal oscillation. We model the exposure prediction function as a fully convolutional neural network that can be trained through Gaussian policy gradient in an end-to-end fashion. As a result, our system can associate scene semantics with exposure values; it can also be extended to personalize the exposure adjustments for a user and device. We improve the learning performance by incorporating an adaptive metering module that links semantics with exposure. This adaptive metering module generalizes the conventional spot or matrix metering techniques. We validate our system using the MIT FiveK and our own datasets captured using iPhone 7 and Google Pixel. Experimental results show that our system exhibits stable real-time behavior while improving visual quality compared to what is achieved through native camera control.
cs.CV
we propose a reinforcement learning approach for realtime exposure control of a mobile camera that is personalizable our approach is based on markov decision process mdp in the camera viewfinder or live preview mode given the current frame our system predicts the change in exposure so as to optimize the tradeoff among image quality fast convergence and minimal temporal oscillation we model the exposure prediction function as a fully convolutional neural network that can be trained through gaussian policy gradient in an endtoend fashion as a result our system can associate scene semantics with exposure values it can also be extended to personalize the exposure adjustments for a user and device we improve the learning performance by incorporating an adaptive metering module that links semantics with exposure this adaptive metering module generalizes the conventional spot or matrix metering techniques we validate our system using the mit fivek and our own datasets captured using iphone 7 and google pixel experimental results show that our system exhibits stable realtime behavior while improving visual quality compared to what is achieved through native camera control
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1,803.0227
Revisiting Frequency Moment Estimation in Random Order Streams
We revisit one of the classic problems in the data stream literature, namely, that of estimating the frequency moments $F_p$ for $0 < p < 2$ of an underlying $n$-dimensional vector presented as a sequence of additive updates in a stream. It is well-known that using $p$-stable distributions one can approximate any of these moments up to a multiplicative $(1+\epsilon)$-factor using $O(\epsilon^{-2} \log n)$ bits of space, and this space bound is optimal up to a constant factor in the turnstile streaming model. We show that surprisingly, if one instead considers the popular random-order model of insertion-only streams, in which the updates to the underlying vector arrive in a random order, then one can beat this space bound and achieve $\tilde{O}(\epsilon^{-2} + \log n)$ bits of space, where the $\tilde{O}$ hides poly$(\log(1/\epsilon) + \log \log n)$ factors. If $\epsilon^{-2} \approx \log n$, this represents a roughly quadratic improvement in the space achievable in turnstile streams. Our algorithm is in fact deterministic, and we show our space bound is optimal up to poly$(\log(1/\epsilon) + \log \log n)$ factors for deterministic algorithms in the random order model. We also obtain a similar improvement in space for $p = 2$ whenever $F_2 \gtrsim \log n\cdot F_1$.
cs.DS
we revisit one of the classic problems in the data stream literature namely that of estimating the frequency moments f_p for 0 p 2 of an underlying ndimensional vector presented as a sequence of additive updates in a stream it is wellknown that using pstable distributions one can approximate any of these moments up to a multiplicative 1epsilonfactor using oepsilon2 log n bits of space and this space bound is optimal up to a constant factor in the turnstile streaming model we show that surprisingly if one instead considers the popular randomorder model of insertiononly streams in which the updates to the underlying vector arrive in a random order then one can beat this space bound and achieve tildeoepsilon2 log n bits of space where the tildeo hides polylog1epsilon log log n factors if epsilon2 approx log n this represents a roughly quadratic improvement in the space achievable in turnstile streams our algorithm is in fact deterministic and we show our space bound is optimal up to polylog1epsilon log log n factors for deterministic algorithms in the random order model we also obtain a similar improvement in space for p 2 whenever f_2 gtrsim log ncdot f_1
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1,803.02271
Gravitational Waves produced by Compressible MHD Turbulence from Cosmological Phase Transitions
We calculate the gravitational wave spectrum produced by magneto-hydrodynamic turbulence in a first order phase transitions. We focus in particular on the role of decorrelation of incompressible (solenoidal) homogeneous isotropic turbulence, which is dominated by the sweeping effect. The sweeping effect describes that turbulent decorrelation is primarily due to the small scale eddies being swept with by large scale eddies in a stochastic manner. This effect reduces the gravitational wave signal produced by incompressible MHD turbulence by around an order of magnitude compared to previous studies. Additionally, we find a more complicated dependence for the spectral shape of the gravitational wave spectrum on the energy density sourced by solenoidal modes (magnetic and kinetic). The high frequency tail follows either a $k^{-5/3}$ or a $k^{-8/3}$ power law for large and small solenoidal turbulence density parameter, respectively. Further, magnetic helicity tends to increase the gravitational wave energy at low frequencies. Moreover, we show how solenoidal modes might impact the gravitational wave spectrum from dilatational modes e.g. sound waves. We find that solenoidal modes greatly affect the shape of the gravitational wave spectrum due to the sweeping effect on the dilatational modes. For a high velocity flow, one expects a $k^{-2}$ high frequency tail, due to sweeping. In contrast, for a low velocity flow and a sound wave dominated flow, we expect a $k^{-3}$ high frequency tail. If neither of these limiting cases is realized, the gravitational wave spectrum may be a broken power law with index between -2 and -3, extending up to the frequency at which the source is damped by viscous dissipation.
astro-ph.CO gr-qc
we calculate the gravitational wave spectrum produced by magnetohydrodynamic turbulence in a first order phase transitions we focus in particular on the role of decorrelation of incompressible solenoidal homogeneous isotropic turbulence which is dominated by the sweeping effect the sweeping effect describes that turbulent decorrelation is primarily due to the small scale eddies being swept with by large scale eddies in a stochastic manner this effect reduces the gravitational wave signal produced by incompressible mhd turbulence by around an order of magnitude compared to previous studies additionally we find a more complicated dependence for the spectral shape of the gravitational wave spectrum on the energy density sourced by solenoidal modes magnetic and kinetic the high frequency tail follows either a k53 or a k83 power law for large and small solenoidal turbulence density parameter respectively further magnetic helicity tends to increase the gravitational wave energy at low frequencies moreover we show how solenoidal modes might impact the gravitational wave spectrum from dilatational modes eg sound waves we find that solenoidal modes greatly affect the shape of the gravitational wave spectrum due to the sweeping effect on the dilatational modes for a high velocity flow one expects a k2 high frequency tail due to sweeping in contrast for a low velocity flow and a sound wave dominated flow we expect a k3 high frequency tail if neither of these limiting cases is realized the gravitational wave spectrum may be a broken power law with index between 2 and 3 extending up to the frequency at which the source is damped by viscous dissipation
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1,803.02272
A geometric view of Biodiversity: scaling to metagenomics
We have designed a new efficient dimensionality reduction algorithm in order to investigate new ways of accurately characterizing the biodiversity, namely from a geometric point of view, scaling with large environmental sets produced by NGS ($\sim 10^5$ sequences). The approach is based on Multidimensional Scaling (MDS) that allows for mapping items on a set of $n$ points into a low dimensional euclidean space given the set of pairwise distances. We compute all pairwise distances between reads in a given sample, run MDS on the distance matrix, and analyze the projection on first axis, by visualization tools. We have circumvented the quadratic complexity of computing pairwise distances by implementing it on a hyperparallel computer (Turing, a Blue Gene Q), and the cubic complexity of the spectral decomposition by implementing a dense random projection based algorithm. We have applied this data analysis scheme on a set of $10^5$ reads, which are amplicons of a diatom environmental sample from Lake Geneva. Analyzing the shape of the point cloud paves the way for a geometric analysis of biodiversity, and for accurately building OTUs (Operational Taxonomic Units), when the data set is too large for implementing unsupervised, hierarchical, high-dimensional clustering.
stat.CO q-bio.QM
we have designed a new efficient dimensionality reduction algorithm in order to investigate new ways of accurately characterizing the biodiversity namely from a geometric point of view scaling with large environmental sets produced by ngs sim 105 sequences the approach is based on multidimensional scaling mds that allows for mapping items on a set of n points into a low dimensional euclidean space given the set of pairwise distances we compute all pairwise distances between reads in a given sample run mds on the distance matrix and analyze the projection on first axis by visualization tools we have circumvented the quadratic complexity of computing pairwise distances by implementing it on a hyperparallel computer turing a blue gene q and the cubic complexity of the spectral decomposition by implementing a dense random projection based algorithm we have applied this data analysis scheme on a set of 105 reads which are amplicons of a diatom environmental sample from lake geneva analyzing the shape of the point cloud paves the way for a geometric analysis of biodiversity and for accurately building otus operational taxonomic units when the data set is too large for implementing unsupervised hierarchical highdimensional clustering
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1,803.02273
Dissonant points and the region of influence of non-saddle sets
The aim of this paper is to study dynamical and topological properties of a flow in the region of influence of an isolated non-saddle set. We see, in particular, that some topological conditions are sufficient to guarantee that these sets are attractors or repellers. We study in detail the existence of dissonant points of the flow, which play a key role in the description of the region of influence of a non-saddle set. These points are responsible for much of the dynamical and topological complexity of the system. We also study non-saddle sets from the point of view of the Conley index theory and consider, among other things, the case of flows on manifolds with trivial first cohomology group. For flows on these manifolds, dynamical robustness is equivalent to topological robustness. We carry out a particular study of 2-dimensional flows and give a topological condition which detects the existence of dissonant points for flows on surfaces. We also prove that isolated invariant continua of planar flows with global region of influence are necessarily attractors or repellers.
math.DS
the aim of this paper is to study dynamical and topological properties of a flow in the region of influence of an isolated nonsaddle set we see in particular that some topological conditions are sufficient to guarantee that these sets are attractors or repellers we study in detail the existence of dissonant points of the flow which play a key role in the description of the region of influence of a nonsaddle set these points are responsible for much of the dynamical and topological complexity of the system we also study nonsaddle sets from the point of view of the conley index theory and consider among other things the case of flows on manifolds with trivial first cohomology group for flows on these manifolds dynamical robustness is equivalent to topological robustness we carry out a particular study of 2dimensional flows and give a topological condition which detects the existence of dissonant points for flows on surfaces we also prove that isolated invariant continua of planar flows with global region of influence are necessarily attractors or repellers
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1,803.02274
Regularity of many-body Schr\"odinger evolution equation and its application to numerical analysis
A decade ago, the mixed regularity of stationary many-body Schr\"o\-dinger equation has been studied by Harry Yserentant through the Pauli Principle and the Hardy inequality (Uncertainty Principle). In this article, we prove that the many-body evolution Schr\"odinger equation has a similar mixed regularity if the initial data $u_0$ satisfies the Pauli Principle. By generalization of the Strichartz estimates, our method also applies to the numerical approximation of this problem: based on these mixed derivatives, we design a new approximation which can hugely improve the computing capability especially in quantum chemistry.
math.AP
a decade ago the mixed regularity of stationary manybody schrodinger equation has been studied by harry yserentant through the pauli principle and the hardy inequality uncertainty principle in this article we prove that the manybody evolution schrodinger equation has a similar mixed regularity if the initial data u_0 satisfies the pauli principle by generalization of the strichartz estimates our method also applies to the numerical approximation of this problem based on these mixed derivatives we design a new approximation which can hugely improve the computing capability especially in quantum chemistry
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1,803.02275
Toposes of connectivity spaces. Morita equivalences with topological spaces and partially ordered sets in the finite case
This paper has two parts. First, we recall and detail the definition of the Grothendieck topos of a connectivity space, that is the topos of sheaves on such a space. In the second part, we prove that every finite connectivity space is Morita-equivalent to a finite topological space, and vice versa (we have given this proof in several, but we haven't yet shared this in writing).
math.GN math.CT
this paper has two parts first we recall and detail the definition of the grothendieck topos of a connectivity space that is the topos of sheaves on such a space in the second part we prove that every finite connectivity space is moritaequivalent to a finite topological space and vice versa we have given this proof in several but we havent yet shared this in writing
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1,803.02276
GeoNet: Unsupervised Learning of Dense Depth, Optical Flow and Camera Pose
We propose GeoNet, a jointly unsupervised learning framework for monocular depth, optical flow and ego-motion estimation from videos. The three components are coupled by the nature of 3D scene geometry, jointly learned by our framework in an end-to-end manner. Specifically, geometric relationships are extracted over the predictions of individual modules and then combined as an image reconstruction loss, reasoning about static and dynamic scene parts separately. Furthermore, we propose an adaptive geometric consistency loss to increase robustness towards outliers and non-Lambertian regions, which resolves occlusions and texture ambiguities effectively. Experimentation on the KITTI driving dataset reveals that our scheme achieves state-of-the-art results in all of the three tasks, performing better than previously unsupervised methods and comparably with supervised ones.
cs.CV
we propose geonet a jointly unsupervised learning framework for monocular depth optical flow and egomotion estimation from videos the three components are coupled by the nature of 3d scene geometry jointly learned by our framework in an endtoend manner specifically geometric relationships are extracted over the predictions of individual modules and then combined as an image reconstruction loss reasoning about static and dynamic scene parts separately furthermore we propose an adaptive geometric consistency loss to increase robustness towards outliers and nonlambertian regions which resolves occlusions and texture ambiguities effectively experimentation on the kitti driving dataset reveals that our scheme achieves stateoftheart results in all of the three tasks performing better than previously unsupervised methods and comparably with supervised ones
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1,803.02277
The interstellar medium: from molecules to star formation
The interstellar medium (ISM) is a very complex medium which contains the matter needed to form stars and planets. The ISM is in permanent interaction with radiation, turbulence, magnetic and gravitational fields, and accelerated particles. Everything that happens in this medium has consequences on the dynamics and evolution of the Galaxy, resulting the link that relates the stellar scale with the galactic one. Thus, the study of the ISM is crucial to advance in the knowledge of stellar and galactic astrophysics. In this article I present a summary of what we know about the physics and chemistry of this medium, giving an special emphasis on star formation, and how the processes related to the stars birth and evolution interrelate with the environment that surrounds them.
astro-ph.GA
the interstellar medium ism is a very complex medium which contains the matter needed to form stars and planets the ism is in permanent interaction with radiation turbulence magnetic and gravitational fields and accelerated particles everything that happens in this medium has consequences on the dynamics and evolution of the galaxy resulting the link that relates the stellar scale with the galactic one thus the study of the ism is crucial to advance in the knowledge of stellar and galactic astrophysics in this article i present a summary of what we know about the physics and chemistry of this medium giving an special emphasis on star formation and how the processes related to the stars birth and evolution interrelate with the environment that surrounds them
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1,803.02278
Trapping and sorting active particles: motility-induced condensation & smectic defects
We present an experimental realization of the collective trapping phase transition [Kaiser et al., PRL 108, 268307 (2012)], using motile polar granular rods in the presence of a V-shaped obstacle. We offer a theory of this transition based on the interplay of motility-induced condensation and liquid-crystalline ordering and show that trapping occurs when persistent influx overcomes the collective expulsion of smectic defect structures. In agreement with the theory, our experiments find that a trap fills to the brim when the trap angle $\theta$ is below a threshold $\theta_c$, while all particles escape for $\theta > \theta_c$. Our simulations support a further prediction, that $\theta_c$ goes down with increasing rotational noise. We exploit the sensitivity of trapping to the persistence of directed motion to sort particles based on the statistical properties of their activity
cond-mat.soft
we present an experimental realization of the collective trapping phase transition kaiser et al prl 108 268307 2012 using motile polar granular rods in the presence of a vshaped obstacle we offer a theory of this transition based on the interplay of motilityinduced condensation and liquidcrystalline ordering and show that trapping occurs when persistent influx overcomes the collective expulsion of smectic defect structures in agreement with the theory our experiments find that a trap fills to the brim when the trap angle theta is below a threshold theta_c while all particles escape for theta theta_c our simulations support a further prediction that theta_c goes down with increasing rotational noise we exploit the sensitivity of trapping to the persistence of directed motion to sort particles based on the statistical properties of their activity
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1,803.02279
An End-to-End Goal-Oriented Dialog System with a Generative Natural Language Response Generation
Recently advancements in deep learning allowed the development of end-to-end trained goal-oriented dialog systems. Although these systems already achieve good performance, some simplifications limit their usage in real-life scenarios. In this work, we address two of these limitations: ignoring positional information and a fixed number of possible response candidates. We propose to use positional encodings in the input to model the word order of the user utterances. Furthermore, by using a feedforward neural network, we are able to generate the output word by word and are no longer restricted to a fixed number of possible response candidates. Using the positional encoding, we were able to achieve better accuracies in the Dialog bAbI Tasks and using the feedforward neural network for generating the response, we were able to save computation time and space consumption.
cs.CL
recently advancements in deep learning allowed the development of endtoend trained goaloriented dialog systems although these systems already achieve good performance some simplifications limit their usage in reallife scenarios in this work we address two of these limitations ignoring positional information and a fixed number of possible response candidates we propose to use positional encodings in the input to model the word order of the user utterances furthermore by using a feedforward neural network we are able to generate the output word by word and are no longer restricted to a fixed number of possible response candidates using the positional encoding we were able to achieve better accuracies in the dialog babi tasks and using the feedforward neural network for generating the response we were able to save computation time and space consumption
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1,803.0228
ART-UP: A Novel Method for Generating Scanning-robust Aesthetic QR codes
QR codes are usually scanned in different environments, so they must be robust to variations in illumination, scale, coverage, and camera angles. Aesthetic QR codes improve the visual quality, but subtle changes in their appearance may cause scanning failure. In this paper, a new method to generate scanning-robust aesthetic QR codes is proposed, which is based on a module-based scanning probability estimation model that can effectively balance the tradeoff between visual quality and scanning robustness. Our method locally adjusts the luminance of each module by estimating the probability of successful sampling. The approach adopts the hierarchical, coarse-to-fine strategy to enhance the visual quality of aesthetic QR codes, which sequentially generate the following three codes: a binary aesthetic QR code, a grayscale aesthetic QR code, and the final color aesthetic QR code. Our approach also can be used to create QR codes with different visual styles by adjusting some initialization parameters. User surveys and decoding experiments were adopted for evaluating our method compared with state-of-the-art algorithms, which indicates that the proposed approach has excellent performance in terms of both visual quality and scanning robustness.
cs.MM
qr codes are usually scanned in different environments so they must be robust to variations in illumination scale coverage and camera angles aesthetic qr codes improve the visual quality but subtle changes in their appearance may cause scanning failure in this paper a new method to generate scanningrobust aesthetic qr codes is proposed which is based on a modulebased scanning probability estimation model that can effectively balance the tradeoff between visual quality and scanning robustness our method locally adjusts the luminance of each module by estimating the probability of successful sampling the approach adopts the hierarchical coarsetofine strategy to enhance the visual quality of aesthetic qr codes which sequentially generate the following three codes a binary aesthetic qr code a grayscale aesthetic qr code and the final color aesthetic qr code our approach also can be used to create qr codes with different visual styles by adjusting some initialization parameters user surveys and decoding experiments were adopted for evaluating our method compared with stateoftheart algorithms which indicates that the proposed approach has excellent performance in terms of both visual quality and scanning robustness
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1,803.02281
High Precision Statistical Landau Gauge Lattice Gluon Propagator Computation vs. the Gribov-Zwanziger approach
The compatibility of the results from the Gribov-Zwanziger tree level prediction and lattice simulations, using large statistical ensembles, for the Landau gauge gluon propagator are investigated, thereby complementing earlier work using small-scale statistics. Our results show that the data is well described by the tree level estimate only up to momenta $p \lesssim 1$ GeV while clearly favoring the so-called Refined Gribov-Zwanziger scenario, implying particular relations between certain possible $d=2$ condensates. We also provide a global fit of the lattice data which interpolates between the above scenario at low momenta and the usual continuum one-loop renormalization improved perturbation theory after introducing an infrared log-regularizing term.
hep-lat hep-ph hep-th nucl-th
the compatibility of the results from the gribovzwanziger tree level prediction and lattice simulations using large statistical ensembles for the landau gauge gluon propagator are investigated thereby complementing earlier work using smallscale statistics our results show that the data is well described by the tree level estimate only up to momenta p lesssim 1 gev while clearly favoring the socalled refined gribovzwanziger scenario implying particular relations between certain possible d2 condensates we also provide a global fit of the lattice data which interpolates between the above scenario at low momenta and the usual continuum oneloop renormalization improved perturbation theory after introducing an infrared logregularizing term
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1,803.02282
The Preeminence of Ethnic Diversity in Scientific Collaboration
Inspired by the social and economic benefits of diversity, we analyze over 9 million papers and 6 million scientists to study the relationship between research impact and five classes of diversity: ethnicity, discipline, gender, affiliation, and academic age. Using randomized baseline models, we establish the presence of homophily in ethnicity, gender and affiliation. We then study the effect of diversity on scientific impact, as reflected in citations. Remarkably, of the classes considered, ethnic diversity had the strongest correlation with scientific impact. To further isolate the effects of ethnic diversity, we used randomized baseline models and again found a clear link between diversity and impact. To further support these findings, we use coarsened exact matching to compare the scientific impact of ethnically diverse papers and scientists with closely-matched control groups. Here, we find that ethnic diversity resulted in an impact gain of 10.63% for papers, and 47.67% for scientists.
cs.DL cs.SI physics.soc-ph
inspired by the social and economic benefits of diversity we analyze over 9 million papers and 6 million scientists to study the relationship between research impact and five classes of diversity ethnicity discipline gender affiliation and academic age using randomized baseline models we establish the presence of homophily in ethnicity gender and affiliation we then study the effect of diversity on scientific impact as reflected in citations remarkably of the classes considered ethnic diversity had the strongest correlation with scientific impact to further isolate the effects of ethnic diversity we used randomized baseline models and again found a clear link between diversity and impact to further support these findings we use coarsened exact matching to compare the scientific impact of ethnically diverse papers and scientists with closelymatched control groups here we find that ethnic diversity resulted in an impact gain of 1063 for papers and 4767 for scientists
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1,803.02283
Effect of charge ordering on the electrical properties and magnetoresistance of manganites
The Monte Carlo Ferromagnetic Ising model was used to study the electrical properties of manganese oxides due to the charge ordering phase occurring at doping, x = 0.5. The half-doped manganites have an insulator antiferromagnetic ground state. We calculated the internal energy, specific heat, resistivity and the magneto-resistance, MR, with parallel and anti-parallel applied magnetic fields. Our simulation reveals that the resistivity decreases exponentially and the electric current increases with increasing temperature according the free charge increase, to transport from an insulator to conductor phase. The magnetoresistance has negative small values with parallel magnetic field but has positive high values with unti-parallel magnetic field. The obtained semiconductor-metal transition behavior candidates the half-doped manganites to be very good semiconductors diode junctions.
cond-mat.str-el
the monte carlo ferromagnetic ising model was used to study the electrical properties of manganese oxides due to the charge ordering phase occurring at doping x 05 the halfdoped manganites have an insulator antiferromagnetic ground state we calculated the internal energy specific heat resistivity and the magnetoresistance mr with parallel and antiparallel applied magnetic fields our simulation reveals that the resistivity decreases exponentially and the electric current increases with increasing temperature according the free charge increase to transport from an insulator to conductor phase the magnetoresistance has negative small values with parallel magnetic field but has positive high values with untiparallel magnetic field the obtained semiconductormetal transition behavior candidates the halfdoped manganites to be very good semiconductors diode junctions
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1,803.02284
Zero-Shot Sketch-Image Hashing
Recent studies show that large-scale sketch-based image retrieval (SBIR) can be efficiently tackled by cross-modal binary representation learning methods, where Hamming distance matching significantly speeds up the process of similarity search. Providing training and test data subjected to a fixed set of pre-defined categories, the cutting-edge SBIR and cross-modal hashing works obtain acceptable retrieval performance. However, most of the existing methods fail when the categories of query sketches have never been seen during training. In this paper, the above problem is briefed as a novel but realistic zero-shot SBIR hashing task. We elaborate the challenges of this special task and accordingly propose a zero-shot sketch-image hashing (ZSIH) model. An end-to-end three-network architecture is built, two of which are treated as the binary encoders. The third network mitigates the sketch-image heterogeneity and enhances the semantic relations among data by utilizing the Kronecker fusion layer and graph convolution, respectively. As an important part of ZSIH, we formulate a generative hashing scheme in reconstructing semantic knowledge representations for zero-shot retrieval. To the best of our knowledge, ZSIH is the first zero-shot hashing work suitable for SBIR and cross-modal search. Comprehensive experiments are conducted on two extended datasets, i.e., Sketchy and TU-Berlin with a novel zero-shot train-test split. The proposed model remarkably outperforms related works.
cs.CV
recent studies show that largescale sketchbased image retrieval sbir can be efficiently tackled by crossmodal binary representation learning methods where hamming distance matching significantly speeds up the process of similarity search providing training and test data subjected to a fixed set of predefined categories the cuttingedge sbir and crossmodal hashing works obtain acceptable retrieval performance however most of the existing methods fail when the categories of query sketches have never been seen during training in this paper the above problem is briefed as a novel but realistic zeroshot sbir hashing task we elaborate the challenges of this special task and accordingly propose a zeroshot sketchimage hashing zsih model an endtoend threenetwork architecture is built two of which are treated as the binary encoders the third network mitigates the sketchimage heterogeneity and enhances the semantic relations among data by utilizing the kronecker fusion layer and graph convolution respectively as an important part of zsih we formulate a generative hashing scheme in reconstructing semantic knowledge representations for zeroshot retrieval to the best of our knowledge zsih is the first zeroshot hashing work suitable for sbir and crossmodal search comprehensive experiments are conducted on two extended datasets ie sketchy and tuberlin with a novel zeroshot traintest split the proposed model remarkably outperforms related works
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1,803.02285
Hybrid Multi-camera Visual Servoing to Moving Target
Visual servoing is a well-known task in robotics. However, there are still challenges when multiple visual sources are combined to accurately guide the robot or occlusions appear. In this paper we present a novel visual servoing approach using hybrid multi-camera input data to lead a robot arm accurately to dynamically moving target points in the presence of partial occlusions. The approach uses four RGBD sensors as Eye-to-Hand (EtoH) visual input, and an arm-mounted stereo camera as Eye-in-Hand (EinH). A Master supervisor task selects between using the EtoH or the EinH, depending on the distance between the robot and target. The Master also selects the subset of EtoH cameras that best perceive the target. When the EinH sensor is used, if the target becomes occluded or goes out of the sensor's view-frustum, the Master switches back to the EtoH sensors to re-track the object. Using this adaptive visual input data, the robot is then controlled using an iterative planner that uses position, orientation and joint configuration to estimate the trajectory. Since the target is dynamic, this trajectory is updated every time-step. Experiments show good performance in four different situations: tracking a ball, targeting a bulls-eye, guiding a straw to a mouth and delivering an item to a moving hand. The experiments cover both simple situations such as a ball that is mostly visible from all cameras, and more complex situations such as the mouth which is partially occluded from some of the sensors.
cs.CV cs.RO
visual servoing is a wellknown task in robotics however there are still challenges when multiple visual sources are combined to accurately guide the robot or occlusions appear in this paper we present a novel visual servoing approach using hybrid multicamera input data to lead a robot arm accurately to dynamically moving target points in the presence of partial occlusions the approach uses four rgbd sensors as eyetohand etoh visual input and an armmounted stereo camera as eyeinhand einh a master supervisor task selects between using the etoh or the einh depending on the distance between the robot and target the master also selects the subset of etoh cameras that best perceive the target when the einh sensor is used if the target becomes occluded or goes out of the sensors viewfrustum the master switches back to the etoh sensors to retrack the object using this adaptive visual input data the robot is then controlled using an iterative planner that uses position orientation and joint configuration to estimate the trajectory since the target is dynamic this trajectory is updated every timestep experiments show good performance in four different situations tracking a ball targeting a bullseye guiding a straw to a mouth and delivering an item to a moving hand the experiments cover both simple situations such as a ball that is mostly visible from all cameras and more complex situations such as the mouth which is partially occluded from some of the sensors
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1,803.02286
Learning monocular visual odometry with dense 3D mapping from dense 3D flow
This paper introduces a fully deep learning approach to monocular SLAM, which can perform simultaneous localization using a neural network for learning visual odometry (L-VO) and dense 3D mapping. Dense 2D flow and a depth image are generated from monocular images by sub-networks, which are then used by a 3D flow associated layer in the L-VO network to generate dense 3D flow. Given this 3D flow, the dual-stream L-VO network can then predict the 6DOF relative pose and furthermore reconstruct the vehicle trajectory. In order to learn the correlation between motion directions, the Bivariate Gaussian modelling is employed in the loss function. The L-VO network achieves an overall performance of 2.68% for average translational error and 0.0143 deg/m for average rotational error on the KITTI odometry benchmark. Moreover, the learned depth is fully leveraged to generate a dense 3D map. As a result, an entire visual SLAM system, that is, learning monocular odometry combined with dense 3D mapping, is achieved.
cs.RO cs.CV
this paper introduces a fully deep learning approach to monocular slam which can perform simultaneous localization using a neural network for learning visual odometry lvo and dense 3d mapping dense 2d flow and a depth image are generated from monocular images by subnetworks which are then used by a 3d flow associated layer in the lvo network to generate dense 3d flow given this 3d flow the dualstream lvo network can then predict the 6dof relative pose and furthermore reconstruct the vehicle trajectory in order to learn the correlation between motion directions the bivariate gaussian modelling is employed in the loss function the lvo network achieves an overall performance of 268 for average translational error and 00143 degm for average rotational error on the kitti odometry benchmark moreover the learned depth is fully leveraged to generate a dense 3d map as a result an entire visual slam system that is learning monocular odometry combined with dense 3d mapping is achieved
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1,803.02287
Analyzing the basic principles of tissue microarray data measuring the cooperative phenomena of marker proteins in invasive breast cancer
The analysis of a protein-expression pattern from tissue microarray (TMA) data will not immediately give an answer on synergistic or antagonistic effects between the expression of the observed proteins. But contrary to apparent first impression, it is possible to reveal those cooperative phenomena from TMA data. We present here a largely assumption-free combinatorial analysis, related to correlation networks but with much less arbitrary constraints. A strong focus was put on the analysis of the basic data to analyze how the cooperative phenomena might be imprinted in the TMA data structure. The study design was based on two independent panels of 589 and 366 invasive breast cancer cases from different institutions, assembled on tissue microarrays. The combinatorial analysis generates an optimal rank ordering of protein-expression coherence. The outcome of the analysis corresponds to all the single observations scattered over several publications and integrates them in one context. This means all these scattered observations can also be deduced from one TMA experiment. A comprehensive statistical meta-analysis of the TMA data suggests the existence of a superposition of three basic coherence situations, and offers the opportunity to analyze these data properties with additional real-world data and synthetic data in more detail. The presented algorithm gives molecular pathologists a tool to extract dependency information from TMA data. Beyond this practical benefit, some light was shed on how dependency aspects might be imprinted into expression data. This will certainly foster the refinement of algorithms to reconstruct dependency networks. The implementation of the algorithm is at the moment not end-user suitable, but available on request.
q-bio.MN
the analysis of a proteinexpression pattern from tissue microarray tma data will not immediately give an answer on synergistic or antagonistic effects between the expression of the observed proteins but contrary to apparent first impression it is possible to reveal those cooperative phenomena from tma data we present here a largely assumptionfree combinatorial analysis related to correlation networks but with much less arbitrary constraints a strong focus was put on the analysis of the basic data to analyze how the cooperative phenomena might be imprinted in the tma data structure the study design was based on two independent panels of 589 and 366 invasive breast cancer cases from different institutions assembled on tissue microarrays the combinatorial analysis generates an optimal rank ordering of proteinexpression coherence the outcome of the analysis corresponds to all the single observations scattered over several publications and integrates them in one context this means all these scattered observations can also be deduced from one tma experiment a comprehensive statistical metaanalysis of the tma data suggests the existence of a superposition of three basic coherence situations and offers the opportunity to analyze these data properties with additional realworld data and synthetic data in more detail the presented algorithm gives molecular pathologists a tool to extract dependency information from tma data beyond this practical benefit some light was shed on how dependency aspects might be imprinted into expression data this will certainly foster the refinement of algorithms to reconstruct dependency networks the implementation of the algorithm is at the moment not enduser suitable but available on request
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1,803.02288
A New Scaling Law for Activity Detection in Massive MIMO Systems
In this paper, we study the problem of \textit{activity detection} (AD) in a massive MIMO setup, where the Base Station (BS) has $M \gg 1$ antennas. We consider a block fading channel model where the $M$-dim channel vector of each user remains almost constant over a \textit{coherence block} (CB) containing $D_c$ signal dimensions. We study a setting in which the number of potential users $K_c$ assigned to a specific CB is much larger than the dimension of the CB $D_c$ ($K_c \gg D_c$) but at each time slot only $A_c \ll K_c$ of them are active. Most of the previous results, based on compressed sensing, require that $A_c\le D_c$, which is a bottleneck in massive deployment scenarios such as Internet-of-Things (IoT) and Device-to-Device (D2D) communication. In this paper, we show that one can overcome this fundamental limitation when the number of BS antennas $M$ is sufficiently large. More specifically, we derive a \textit{scaling law} on the parameters $(M, D_c, K_c, A_c)$ and also \textit{Signal-to-Noise Ratio} (SNR) under which our proposed AD scheme succeeds. Our analysis indicates that with a CB of dimension $D_c$, and a sufficient number of BS antennas $M$ with $A_c/M=o(1)$, one can identify the activity of $A_c=O(D_c^2/\log^2(\frac{K_c}{A_c}))$ active users, which is much larger than the previous bound $A_c=O(D_c)$ obtained via traditional compressed sensing techniques. In particular, in our proposed scheme one needs to pay only a poly-logarithmic penalty $O(\log^2(\frac{K_c}{A_c}))$ for increasing the number of potential users $K_c$, which makes it ideally suited for AD in IoT setups. We propose low-complexity algorithms for AD and provide numerical simulations to illustrate our results. We also compare the performance of our proposed AD algorithms with that of other competitive algorithms in the literature.
cs.IT math.IT
in this paper we study the problem of textitactivity detection ad in a massive mimo setup where the base station bs has m gg 1 antennas we consider a block fading channel model where the mdim channel vector of each user remains almost constant over a textitcoherence block cb containing d_c signal dimensions we study a setting in which the number of potential users k_c assigned to a specific cb is much larger than the dimension of the cb d_c k_c gg d_c but at each time slot only a_c ll k_c of them are active most of the previous results based on compressed sensing require that a_cle d_c which is a bottleneck in massive deployment scenarios such as internetofthings iot and devicetodevice d2d communication in this paper we show that one can overcome this fundamental limitation when the number of bs antennas m is sufficiently large more specifically we derive a textitscaling law on the parameters m d_c k_c a_c and also textitsignaltonoise ratio snr under which our proposed ad scheme succeeds our analysis indicates that with a cb of dimension d_c and a sufficient number of bs antennas m with a_cmo1 one can identify the activity of a_cod_c2log2frack_ca_c active users which is much larger than the previous bound a_cod_c obtained via traditional compressed sensing techniques in particular in our proposed scheme one needs to pay only a polylogarithmic penalty olog2frack_ca_c for increasing the number of potential users k_c which makes it ideally suited for ad in iot setups we propose lowcomplexity algorithms for ad and provide numerical simulations to illustrate our results we also compare the performance of our proposed ad algorithms with that of other competitive algorithms in the literature
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1,803.02289
Testing the complexity of a valued CSP language
A Valued Constraint Satisfaction Problem (VCSP) provides a common framework that can express a wide range of discrete optimization problems. A VCSP instance is given by a finite set of variables, a finite domain of labels, and an objective function to be minimized. This function is represented as a sum of terms where each term depends on a subset of the variables. To obtain different classes of optimization problems, one can restrict all terms to come from a fixed set $\Gamma$ of cost functions, called a language. Recent breakthrough results have established a complete complexity classification of such classes with respect to language $\Gamma$: if all cost functions in $\Gamma$ satisfy a certain algebraic condition then all $\Gamma$-instances can be solved in polynomial time, otherwise the problem is NP-hard. Unfortunately, testing this condition for a given language $\Gamma$ is known to be NP-hard. We thus study exponential algorithms for this meta-problem. We show that the tractability condition of a finite-valued language $\Gamma$ can be tested in $O(\sqrt[3]{3}^{\,|D|}\cdot poly(size(\Gamma)))$ time, where $D$ is the domain of $\Gamma$ and $poly(\cdot)$ is some fixed polynomial. We also obtain a matching lower bound under the Strong Exponential Time Hypothesis (SETH). More precisely, we prove that for any constant $\delta<1$ there is no $O(\sqrt[3]{3}^{\,\delta|D|})$ algorithm, assuming that SETH holds.
cs.CC
a valued constraint satisfaction problem vcsp provides a common framework that can express a wide range of discrete optimization problems a vcsp instance is given by a finite set of variables a finite domain of labels and an objective function to be minimized this function is represented as a sum of terms where each term depends on a subset of the variables to obtain different classes of optimization problems one can restrict all terms to come from a fixed set gamma of cost functions called a language recent breakthrough results have established a complete complexity classification of such classes with respect to language gamma if all cost functions in gamma satisfy a certain algebraic condition then all gammainstances can be solved in polynomial time otherwise the problem is nphard unfortunately testing this condition for a given language gamma is known to be nphard we thus study exponential algorithms for this metaproblem we show that the tractability condition of a finitevalued language gamma can be tested in osqrt33dcdot polysizegamma time where d is the domain of gamma and polycdot is some fixed polynomial we also obtain a matching lower bound under the strong exponential time hypothesis seth more precisely we prove that for any constant delta1 there is no osqrt33deltad algorithm assuming that seth holds
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1,803.0229
Bouligand-Landweber iteration for a non-smooth ill-posed problem
This work is concerned with the iterative regularization of a non-smooth nonlinear ill-posed problem where the forward mapping is merely directionally but not G\^ateaux differentiable. Using a Bouligand subderivative of the forward mapping, a modified Landweber method can be applied; however, the standard analysis is not applicable since the Bouligand subderivative mapping is not continuous unless the forward mapping is G\^ateaux differentiable. We therefore provide a novel convergence analysis of the modified Landweber method that is based on the concept of asymptotic stability and merely requires a generalized tangential cone condition. These conditions are verified for an inverse source problem for an elliptic PDE with a non-smooth Lipschitz continuous nonlinearity, showing that the corresponding Bouligand--Landweber iteration converges strongly for exact data as well as in the limit of vanishing data if the iteration is stopped according to the discrepancy principle. This is illustrated
math.NA math.OC
this work is concerned with the iterative regularization of a nonsmooth nonlinear illposed problem where the forward mapping is merely directionally but not gateaux differentiable using a bouligand subderivative of the forward mapping a modified landweber method can be applied however the standard analysis is not applicable since the bouligand subderivative mapping is not continuous unless the forward mapping is gateaux differentiable we therefore provide a novel convergence analysis of the modified landweber method that is based on the concept of asymptotic stability and merely requires a generalized tangential cone condition these conditions are verified for an inverse source problem for an elliptic pde with a nonsmooth lipschitz continuous nonlinearity showing that the corresponding bouligandlandweber iteration converges strongly for exact data as well as in the limit of vanishing data if the iteration is stopped according to the discrepancy principle this is illustrated
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1,803.02291
Synthesizing Neural Network Controllers with Probabilistic Model based Reinforcement Learning
We present an algorithm for rapidly learning controllers for robotics systems. The algorithm follows the model-based reinforcement learning paradigm, and improves upon existing algorithms; namely Probabilistic learning in Control (PILCO) and a sample-based version of PILCO with neural network dynamics (Deep-PILCO). We propose training a neural network dynamics model using variational dropout with truncated Log-Normal noise. This allows us to obtain a dynamics model with calibrated uncertainty, which can be used to simulate controller executions via rollouts. We also describe set of techniques, inspired by viewing PILCO as a recurrent neural network model, that are crucial to improve the convergence of the method. We test our method on a variety of benchmark tasks, demonstrating data-efficiency that is competitive with PILCO, while being able to optimize complex neural network controllers. Finally, we assess the performance of the algorithm for learning motor controllers for a six legged autonomous underwater vehicle. This demonstrates the potential of the algorithm for scaling up the dimensionality and dataset sizes, in more complex control tasks.
cs.RO cs.AI
we present an algorithm for rapidly learning controllers for robotics systems the algorithm follows the modelbased reinforcement learning paradigm and improves upon existing algorithms namely probabilistic learning in control pilco and a samplebased version of pilco with neural network dynamics deeppilco we propose training a neural network dynamics model using variational dropout with truncated lognormal noise this allows us to obtain a dynamics model with calibrated uncertainty which can be used to simulate controller executions via rollouts we also describe set of techniques inspired by viewing pilco as a recurrent neural network model that are crucial to improve the convergence of the method we test our method on a variety of benchmark tasks demonstrating dataefficiency that is competitive with pilco while being able to optimize complex neural network controllers finally we assess the performance of the algorithm for learning motor controllers for a six legged autonomous underwater vehicle this demonstrates the potential of the algorithm for scaling up the dimensionality and dataset sizes in more complex control tasks
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1,803.02292
Weak Decays of Heavy Baryons in Light-Front Approach
In this work, we perform a analysis of semi-leptonic and nonleptonic weak decays of heavy baryons: $\Lambda_{b},\Xi_{b},\Omega_{b}$ and $\Lambda_{c},\Xi_{c},\Omega_{c}$. For nonleptonic decay modes, we study only the factorizable channels induced by the external W-emission. The two spectator quarks in baryonic transitions are treated as a diquark and form factors are calculated in the light-front approach. Using the results for form factors, we also calculate some corresponding semi-leptonic and nonleptonic decay widths. We find that our results are comparable with the available experimental data and other theoretical predictions. Decay branching fractions for many channels are found to reach the level $10^{-3}\sim10^{-2}$, which are promising to be discovered in the future measurements at BESIII, LHCb and BelleII. The SU(3) symmetry in semi-leptonic decays is examined and sources of symmetry breaking are discussed.
hep-ph hep-ex
in this work we perform a analysis of semileptonic and nonleptonic weak decays of heavy baryons lambda_bxi_bomega_b and lambda_cxi_comega_c for nonleptonic decay modes we study only the factorizable channels induced by the external wemission the two spectator quarks in baryonic transitions are treated as a diquark and form factors are calculated in the lightfront approach using the results for form factors we also calculate some corresponding semileptonic and nonleptonic decay widths we find that our results are comparable with the available experimental data and other theoretical predictions decay branching fractions for many channels are found to reach the level 103sim102 which are promising to be discovered in the future measurements at besiii lhcb and belleii the su3 symmetry in semileptonic decays is examined and sources of symmetry breaking are discussed
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1,803.02293
Pinning Transition of Bose-Einstein Condensates in Optical Ring Resonators
We experimentally investigate the dynamic instability of Bose-Einstein condensates in an optical ring resonator that is asymmetrically pumped in both directions. We find that, beyond a critical resonator-pump detuning, the system becomes stable regardless of the pump strength. Phase diagrams and quenching curves are presented and described by numerical simulations. We discuss a physical explanation based on a geometric interpretation of the underlying nonlinear equations of motion.
physics.atom-ph cond-mat.quant-gas physics.optics
we experimentally investigate the dynamic instability of boseeinstein condensates in an optical ring resonator that is asymmetrically pumped in both directions we find that beyond a critical resonatorpump detuning the system becomes stable regardless of the pump strength phase diagrams and quenching curves are presented and described by numerical simulations we discuss a physical explanation based on a geometric interpretation of the underlying nonlinear equations of motion
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1,803.02294
A self-contained, brief and complete formulation of Voevodsky's Univalence Axiom
In introductions to the subject for a general audience of mathematicians or logicians, the univalence axiom is typically explained by handwaving. This gives rise to several misconceptions, which cannot be properly addressed in the absence of a precise definition. In this short set of notes we give a complete formulation of the univalence axiom from scratch. The underlying idea of these notes is that they should be as concise as possible (and not more). They are not meant to be an Encyclopedia of Univalence.
math.LO
in introductions to the subject for a general audience of mathematicians or logicians the univalence axiom is typically explained by handwaving this gives rise to several misconceptions which cannot be properly addressed in the absence of a precise definition in this short set of notes we give a complete formulation of the univalence axiom from scratch the underlying idea of these notes is that they should be as concise as possible and not more they are not meant to be an encyclopedia of univalence
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1,803.02295
Methods for preparation and detection of neutron spin-orbit states
The generation and control of neutron orbital angular momentum (OAM) states and spin correlated OAM (spin-orbit) states provides a powerful probe of materials with unique penetrating abilities and magnetic sensitivity. We describe techniques to prepare and characterize neutron spin-orbit states, and provide a quantitative comparison to known procedures. The proposed detection method directly measures the correlations of spin state and transverse momentum, and overcomes the major challenges associated with neutrons, which are low flux and small spatial coherence length. Our preparation techniques, utilizing special geometries of magnetic fields, are based on coherent averaging and spatial control methods borrowed from nuclear magnetic resonance. The described procedures may be extended to other probes such as electrons and electromagnetic waves.
quant-ph physics.atom-ph physics.optics
the generation and control of neutron orbital angular momentum oam states and spin correlated oam spinorbit states provides a powerful probe of materials with unique penetrating abilities and magnetic sensitivity we describe techniques to prepare and characterize neutron spinorbit states and provide a quantitative comparison to known procedures the proposed detection method directly measures the correlations of spin state and transverse momentum and overcomes the major challenges associated with neutrons which are low flux and small spatial coherence length our preparation techniques utilizing special geometries of magnetic fields are based on coherent averaging and spatial control methods borrowed from nuclear magnetic resonance the described procedures may be extended to other probes such as electrons and electromagnetic waves
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1,803.02296
State tracking of linear ensembles via optimal mass transport
We consider the problems of tracking an ensemble of indistinguishable agents with linear dynamics based only on output measurements. In this setting, the dynamics of the agents can be modeled by distribution flows in the state space and the measurements correspond to distributions in the output space. In this paper we formulate the corresponding state estimation problem using optimal mass transport theory with prior linear dynamics, and the optimal solution gives an estimate of the state trajectories of the ensemble. For general distributions of systems this can be formulated as a convex optimization problem which is computationally feasible with when the number of state dimensions is low. In the case where the marginal distributions are Gaussian, the problem is reformulated as a semidefinite programming and can be efficiently solved for tracking systems with a large number of states.
cs.SY math.DS
we consider the problems of tracking an ensemble of indistinguishable agents with linear dynamics based only on output measurements in this setting the dynamics of the agents can be modeled by distribution flows in the state space and the measurements correspond to distributions in the output space in this paper we formulate the corresponding state estimation problem using optimal mass transport theory with prior linear dynamics and the optimal solution gives an estimate of the state trajectories of the ensemble for general distributions of systems this can be formulated as a convex optimization problem which is computationally feasible with when the number of state dimensions is low in the case where the marginal distributions are gaussian the problem is reformulated as a semidefinite programming and can be efficiently solved for tracking systems with a large number of states
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1,803.02297
Exponential stabilization of a smart piezoelectric composite beam with only one boundary controller
Layered smart composite beams involving a piezoelectric layer are traditionally actuated by a voltage source by the extension mechanism. In this paper, we consider only the bending and shear of a cantilevered piezoelectric smart composite beam modeled by the Mead-Marcus sandwich beam assumptions. Uniform exponential stabilitization with only one boundary state feedback controller, simultaneously controlling both bending moment and shear, is proved by using a spectral multiplier approach. The state feedback controller slightly differs from the classical counterparts by a non-trivial compact and nonnegative integral operator. This is due to the strong coupling of the charge equation with the stretching and bending equations. For simulations, the so-called filtered semi-discrete finite difference scheme is adopted.
math.AP
layered smart composite beams involving a piezoelectric layer are traditionally actuated by a voltage source by the extension mechanism in this paper we consider only the bending and shear of a cantilevered piezoelectric smart composite beam modeled by the meadmarcus sandwich beam assumptions uniform exponential stabilitization with only one boundary state feedback controller simultaneously controlling both bending moment and shear is proved by using a spectral multiplier approach the state feedback controller slightly differs from the classical counterparts by a nontrivial compact and nonnegative integral operator this is due to the strong coupling of the charge equation with the stretching and bending equations for simulations the socalled filtered semidiscrete finite difference scheme is adopted
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1,803.02298
The CMB neutrino mass / vacuum energy degeneracy: a simple derivation of the degeneracy slopes
It is well known that estimating cosmological parameters from cosmic microwave background (CMB) data alone results in a significant degeneracy between the total neutrino mass and several other cosmological parameters, especially the Hubble constant H_0 and the matter density parameter $\Omega_m$. Adding low-redshift measurements such as baryon acoustic oscillations (BAOs) breaks this degeneracy and greatly improves the constraints on neutrino mass. The sensitivity is surprisingly high, e.g. adding the $\sim 1$ percent measurement of the BAO ratio $r_s/D_V$ from the BOSS survey leads to a limit $\Sigma m_\nu < 0.19$ eV, equivalent to $\Omega_\nu < 0.0045$ at 95\% confidence. For the case of $\Sigma m_\nu < 0.6$ eV, the CMB degeneracy with neutrino mass almost follows a track of constant sound horizon angle (Howlett et al 2012). For a $\Lambda$CDM + $m_\nu$ model, we use simple but quite accurate analytic approximations to derive the slope of this track, giving dimensionless multipliers between the neutrino to matter ratio ($x_\nu \equiv \omega_\nu / \omega_{cb}$) and the shifts in other cosmological parameters. The resulting multipliers are substantially larger than 1: conserving the CMB sound horizon angle requires parameter shifts $\delta \ln H_0 \approx -2 \,\delta x_\nu$, $\delta \ln \Omega_m \approx +5 \, \delta x_\nu$, $\delta \ln \omega_\Lambda \approx -6.2 \, \delta x_\nu$, and most notably $\delta \omega_\Lambda \approx -14 \, \delta \omega_\nu$. These multipliers give an intuitive derivation of the degeneracy direction, which agrees well with the numerical likelihood results from the Planck team.
astro-ph.CO hep-ph
it is well known that estimating cosmological parameters from cosmic microwave background cmb data alone results in a significant degeneracy between the total neutrino mass and several other cosmological parameters especially the hubble constant h_0 and the matter density parameter omega_m adding lowredshift measurements such as baryon acoustic oscillations baos breaks this degeneracy and greatly improves the constraints on neutrino mass the sensitivity is surprisingly high eg adding the sim 1 percent measurement of the bao ratio r_sd_v from the boss survey leads to a limit sigma m_nu 019 ev equivalent to omega_nu 00045 at 95 confidence for the case of sigma m_nu 06 ev the cmb degeneracy with neutrino mass almost follows a track of constant sound horizon angle howlett et al 2012 for a lambdacdm m_nu model we use simple but quite accurate analytic approximations to derive the slope of this track giving dimensionless multipliers between the neutrino to matter ratio x_nu equiv omega_nu omega_cb and the shifts in other cosmological parameters the resulting multipliers are substantially larger than 1 conserving the cmb sound horizon angle requires parameter shifts delta ln h_0 approx 2 delta x_nu delta ln omega_m approx 5 delta x_nu delta ln omega_lambda approx 62 delta x_nu and most notably delta omega_lambda approx 14 delta omega_nu these multipliers give an intuitive derivation of the degeneracy direction which agrees well with the numerical likelihood results from the planck team
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1,803.02299
Spherical collapse and cluster number counts in dark energy models disformally coupled to dark matter
We investigate the effects of a disformal coupling between dark energy and dark matter in the predictions of the spherical collapse and its signatures in galaxy cluster number counts. We find that the disformal coupling has no significant effects on spherical collapse at high redshifts, and in particular during matter domination epoch. However, at lower redshifts, the extrapolated linear density contrast at collapse close to redshift $z \lesssim 1$ and overdensity at virialization can be strongly suppressed by a disformal coupling between dark energy and dark matter. We also find that disformal coupling can have different imprints on cluster number counts compared with conformal coupling, such that the disformal coupling can strongly suppress the predicted number of clusters per redshift interval at $z > 0.1$ while enhance the number of cluster at $z < 0.05$. Using the specifications of eROSITA survey, we find that the disformal coupling between dark energy and dark matter can be tightly constrained by cluster number counts.
astro-ph.CO
we investigate the effects of a disformal coupling between dark energy and dark matter in the predictions of the spherical collapse and its signatures in galaxy cluster number counts we find that the disformal coupling has no significant effects on spherical collapse at high redshifts and in particular during matter domination epoch however at lower redshifts the extrapolated linear density contrast at collapse close to redshift z lesssim 1 and overdensity at virialization can be strongly suppressed by a disformal coupling between dark energy and dark matter we also find that disformal coupling can have different imprints on cluster number counts compared with conformal coupling such that the disformal coupling can strongly suppress the predicted number of clusters per redshift interval at z 01 while enhance the number of cluster at z 005 using the specifications of erosita survey we find that the disformal coupling between dark energy and dark matter can be tightly constrained by cluster number counts
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1,803.023
A Gold Standard for Emotion Annotation in Stack Overflow
Software developers experience and share a wide range of emotions throughout a rich ecosystem of communication channels. A recent trend that has emerged in empirical software engineering studies is leveraging sentiment analysis of developers' communication traces. We release a dataset of 4,800 questions, answers, and comments from Stack Overflow, manually annotated for emotions. Our dataset contributes to the building of a shared corpus of annotated resources to support research on emotion awareness in software development.
cs.SE
software developers experience and share a wide range of emotions throughout a rich ecosystem of communication channels a recent trend that has emerged in empirical software engineering studies is leveraging sentiment analysis of developers communication traces we release a dataset of 4800 questions answers and comments from stack overflow manually annotated for emotions our dataset contributes to the building of a shared corpus of annotated resources to support research on emotion awareness in software development
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1,803.02301
De-Confinement in high multiplicity proton-proton collisions at LHC energies
Recently, the CMS Collaboration has published identified particle transverse momentum spectra in high multiplicity events at LHC energies $\sqrt s $ = 0.9-13 TeV. In the present work the transverse momentum spectra have been analyzed in the framework of the color fields inside the clusters of overlapping strings, which are produced in high energy hadronic collisions. The non-Abelian nature is reflected in the coherence sum of the color fields which as a consequence gives rise to an enhancement of the transverse momentum and a suppression of the multiplicities relative to the non overlapping strings. The initial temperature and shear viscosity to entropy density ratio $\eta/s$ are obtained. For the higher multiplicity events at $\sqrt s $ =7 and 13 TeV the initial temperature is above the universal hadronization temperature and is consistent with the creation of de-confined matter. In these small systems it can be argued that the thermalization is a consequence of the quantum tunneling through the event horizon introduced by the confining color fields, in analogy to the Hawking-Unruh effect. The small shear viscosity to entropy density ratio $\eta/s$ near the critical temperature suggests that the matter is a strongly coupled Quark Gluon Plasma.
hep-ph hep-ex
recently the cms collaboration has published identified particle transverse momentum spectra in high multiplicity events at lhc energies sqrt s 0913 tev in the present work the transverse momentum spectra have been analyzed in the framework of the color fields inside the clusters of overlapping strings which are produced in high energy hadronic collisions the nonabelian nature is reflected in the coherence sum of the color fields which as a consequence gives rise to an enhancement of the transverse momentum and a suppression of the multiplicities relative to the non overlapping strings the initial temperature and shear viscosity to entropy density ratio etas are obtained for the higher multiplicity events at sqrt s 7 and 13 tev the initial temperature is above the universal hadronization temperature and is consistent with the creation of deconfined matter in these small systems it can be argued that the thermalization is a consequence of the quantum tunneling through the event horizon introduced by the confining color fields in analogy to the hawkingunruh effect the small shear viscosity to entropy density ratio etas near the critical temperature suggests that the matter is a strongly coupled quark gluon plasma
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1,803.02302
Randomization inference with general interference and censoring
Interference occurs between individuals when the treatment (or exposure) of one individual affects the outcome of another individual. Previous work on causal inference methods in the presence of interference has focused on the setting where a priori it is assumed there is 'partial interference,' in the sense that individuals can be partitioned into groups wherein there is no interference between individuals in different groups. Bowers, Fredrickson, and Panagopoulos (2012) and Bowers, Fredrickson, and Aronow (2016) consider randomization-based inferential methods that allow for more general interference structures in the context of randomized experiments. In this paper, extensions of Bowers et al. which allow for failure time outcomes subject to right censoring are proposed. Permitting right censored outcomes is challenging because standard randomization-based tests of the null hypothesis of no treatment effect assume that whether an individual is censored does not depend on treatment. The proposed extension of Bowers et al. to allow for censoring entails adapting the method of Wang, Lagakos, and Gray (2010) for two sample survival comparisons in the presence of unequal censoring. The methods are examined via simulation studies and utilized to assess the effects of cholera vaccination in an individually-randomized trial of 73,000 children and women in Matlab, Bangladesh.
stat.ME
interference occurs between individuals when the treatment or exposure of one individual affects the outcome of another individual previous work on causal inference methods in the presence of interference has focused on the setting where a priori it is assumed there is partial interference in the sense that individuals can be partitioned into groups wherein there is no interference between individuals in different groups bowers fredrickson and panagopoulos 2012 and bowers fredrickson and aronow 2016 consider randomizationbased inferential methods that allow for more general interference structures in the context of randomized experiments in this paper extensions of bowers et al which allow for failure time outcomes subject to right censoring are proposed permitting right censored outcomes is challenging because standard randomizationbased tests of the null hypothesis of no treatment effect assume that whether an individual is censored does not depend on treatment the proposed extension of bowers et al to allow for censoring entails adapting the method of wang lagakos and gray 2010 for two sample survival comparisons in the presence of unequal censoring the methods are examined via simulation studies and utilized to assess the effects of cholera vaccination in an individuallyrandomized trial of 73000 children and women in matlab bangladesh
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1,803.02303
Path probabilities for consecutive measurements, and certain "quantum paradoxes"
We consider a finite-dimensional quantum system, making a transition between known initial and final states. The outcomes of several accurate measurements, which {\it could be} made in the interim, define virtual paths, each endowed with a probability amplitude. If the measurements are {\it actually made}, the paths, which may now be called "real", acquire also the probabilities, related to the frequencies, with which a path is seen to be travelled in a series of identical trials. Different sets of measurements, made on the same system, can produce different, or incompatible, statistical ensembles, whose conflicting attributes may, although by no means should, appear "paradoxical". We describe in detail the ensembles, resulting from intermediate measurements of mutually commuting, or non-commuting, operators, in terms of the real paths produced. In the same manner, we analyse the Hardy's and the "three box" paradoxes, the photon's past in an interferometer, the "quantum Cheshire cat" experiment, an the closely related subject of "interaction-free measurements". It is shown that, in all these cases, inaccurate "weak measurements" produce no real paths, and yield only limited information about the virtual paths' probability amplitudes
quant-ph
we consider a finitedimensional quantum system making a transition between known initial and final states the outcomes of several accurate measurements which it could be made in the interim define virtual paths each endowed with a probability amplitude if the measurements are it actually made the paths which may now be called real acquire also the probabilities related to the frequencies with which a path is seen to be travelled in a series of identical trials different sets of measurements made on the same system can produce different or incompatible statistical ensembles whose conflicting attributes may although by no means should appear paradoxical we describe in detail the ensembles resulting from intermediate measurements of mutually commuting or noncommuting operators in terms of the real paths produced in the same manner we analyse the hardys and the three box paradoxes the photons past in an interferometer the quantum cheshire cat experiment an the closely related subject of interactionfree measurements it is shown that in all these cases inaccurate weak measurements produce no real paths and yield only limited information about the virtual paths probability amplitudes
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1,803.02304
Differential Algebras in Codifferential Categories
Differential categories were introduced by Blute, Cockett, and Seely as categorical models of differential linear logic and have since lead to abstract formulations of many notions involving differentiation such as the directional derivative, differential forms, smooth manifolds, De Rham cohomology, etc. In this paper we study the generalization of differential algebras to the context of differential categories by introducing $\mathsf{T}$-differential algebras, which can be seen as special cases of Blute, Lucyshyn-Wright, and O'Neill's notion of $\mathsf{T}$-derivations. As such, $\mathsf{T}$-differential algebras are axiomatized by the chain rule and as a consequence we obtain both the higher-order Leibniz rule and the Fa\`a di Bruno formula for the higher-order chain rule. We also construct both free and cofree $\mathsf{T}$-differential algebras for suitable codifferential categories and discuss power series of $\mathsf{T}$-algebras.
math.CT
differential categories were introduced by blute cockett and seely as categorical models of differential linear logic and have since lead to abstract formulations of many notions involving differentiation such as the directional derivative differential forms smooth manifolds de rham cohomology etc in this paper we study the generalization of differential algebras to the context of differential categories by introducing mathsftdifferential algebras which can be seen as special cases of blute lucyshynwright and oneills notion of mathsftderivations as such mathsftdifferential algebras are axiomatized by the chain rule and as a consequence we obtain both the higherorder leibniz rule and the faa di bruno formula for the higherorder chain rule we also construct both free and cofree mathsftdifferential algebras for suitable codifferential categories and discuss power series of mathsftalgebras
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1,803.02305
Birationally rigid complete intersections of high codimension
We prove that a Fano complete intersection of codimension $k$ and index 1 in the complex projective space ${\mathbb P}^{M+k}$ for $k\geqslant 20$ and $M\geqslant 8k\log k$ with at most multi-quadratic singularities is birationally superrigid. The codimension of the complement to the set of birationally superrigid complete intersections in the natural parameter space is shown to be at least $\frac12 (M-5k)(M-6k)$. The proof is based on the techniques of hypertangent divisors combined with the recently discovered $4n^2$-inequality for complete intersection singularities.
math.AG
we prove that a fano complete intersection of codimension k and index 1 in the complex projective space mathbb pmk for kgeqslant 20 and mgeqslant 8klog k with at most multiquadratic singularities is birationally superrigid the codimension of the complement to the set of birationally superrigid complete intersections in the natural parameter space is shown to be at least frac12 m5km6k the proof is based on the techniques of hypertangent divisors combined with the recently discovered 4n2inequality for complete intersection singularities
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1,803.02306
Toric Nearly K\"ahler manifolds
We show that 6-dimensional strict nearly K\"ahler manifolds admitting effective $\mathbb{T}^3$ actions by automorphisms are completely characterized in the neigbourhood of each point by a function on $\mathbb{R}^3$ satisfying a certain Monge-Amp\`ere type equation.
math.DG
we show that 6dimensional strict nearly kahler manifolds admitting effective mathbbt3 actions by automorphisms are completely characterized in the neigbourhood of each point by a function on mathbbr3 satisfying a certain mongeampere type equation
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1,803.02307
RealPen: Providing Realism in Handwriting Tasks on Touch Surfaces using Auditory-Tactile Feedback
We present RealPen, an augmented stylus for capacitive tablet screens that recreates the physical sensation of writing on paper with a pencil, ball-point pen or marker pen. The aim is to create a more engaging experience when writing on touch surfaces, such as screens of tablet computers. This is achieved by re-generating the friction-induced oscillation and sound of a real writing tool in contact with paper. To generate realistic tactile feedback, our algorithm analyses the frequency spectrum of the friction oscillation generated when writing with traditional tools, extracts principal frequencies, and uses the actuator's frequency response profile for an adjustment weighting function. We enhance the realism by providing the sound feedback aligned with the writing pressure and speed. Furthermore, we investigated the effects of superposition and fluctuation of several frequencies on human tactile perception, evaluated the performance of RealPen, and characterized users' perception and preference of each feedback type.
cs.HC
we present realpen an augmented stylus for capacitive tablet screens that recreates the physical sensation of writing on paper with a pencil ballpoint pen or marker pen the aim is to create a more engaging experience when writing on touch surfaces such as screens of tablet computers this is achieved by regenerating the frictioninduced oscillation and sound of a real writing tool in contact with paper to generate realistic tactile feedback our algorithm analyses the frequency spectrum of the friction oscillation generated when writing with traditional tools extracts principal frequencies and uses the actuators frequency response profile for an adjustment weighting function we enhance the realism by providing the sound feedback aligned with the writing pressure and speed furthermore we investigated the effects of superposition and fluctuation of several frequencies on human tactile perception evaluated the performance of realpen and characterized users perception and preference of each feedback type
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1,803.02308
A Relation between Disorder Chaos and Incongruent States in Spin Glasses on ${\mathbb Z}^d$
We derive lower bounds for the variance of the difference of energies between incongruent ground states, i.e., states with edge overlaps strictly less than one, of the Edwards-Anderson model on ${\mathbb Z}^d$. The bounds highlight a relation between the existence of incongruent ground states and the absence of edge disorder chaos. In particular, it suggests that the presence of disorder chaos is necessary for the variance to be of order less than the volume. In addition, a relation is established between the scale of disorder chaos and the size of critical droplets. The results imply a long-conjectured relation between the droplet theory of Fisher and Huse and the absence of incongruence.
math.PR cond-mat.dis-nn
we derive lower bounds for the variance of the difference of energies between incongruent ground states ie states with edge overlaps strictly less than one of the edwardsanderson model on mathbb zd the bounds highlight a relation between the existence of incongruent ground states and the absence of edge disorder chaos in particular it suggests that the presence of disorder chaos is necessary for the variance to be of order less than the volume in addition a relation is established between the scale of disorder chaos and the size of critical droplets the results imply a longconjectured relation between the droplet theory of fisher and huse and the absence of incongruence
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1,803.02309
Analysing the Potential of BLE to Support Dynamic Broadcasting Scenarios
In this paper, we present a novel approach for broadcasting information based on a Bluetooth Low Energy (BLE) ibeacon technology. We propose a dynamic method that uses a combination of Wi-Fi and BLE technology where every technology plays a part in a user discovery and broadcasting process. In such system, a specific ibeacon device broadcasts the information when a user is in proximity. Using experiments, we conduct a scenario where the system discovers users, disseminates information, and later we use collected data to examine the system performance and capability. The results show that our proposed approach has a promising potential to become a powerful tool in the discovery and broadcasting concept that can be easily implemented and used in business environments.
cs.OH
in this paper we present a novel approach for broadcasting information based on a bluetooth low energy ble ibeacon technology we propose a dynamic method that uses a combination of wifi and ble technology where every technology plays a part in a user discovery and broadcasting process in such system a specific ibeacon device broadcasts the information when a user is in proximity using experiments we conduct a scenario where the system discovers users disseminates information and later we use collected data to examine the system performance and capability the results show that our proposed approach has a promising potential to become a powerful tool in the discovery and broadcasting concept that can be easily implemented and used in business environments
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1,803.0231
Deep Thermal Imaging: Proximate Material Type Recognition in the Wild through Deep Learning of Spatial Surface Temperature Patterns
We introduce Deep Thermal Imaging, a new approach for close-range automatic recognition of materials to enhance the understanding of people and ubiquitous technologies of their proximal environment. Our approach uses a low-cost mobile thermal camera integrated into a smartphone to capture thermal textures. A deep neural network classifies these textures into material types. This approach works effectively without the need for ambient light sources or direct contact with materials. Furthermore, the use of a deep learning network removes the need to handcraft the set of features for different materials. We evaluated the performance of the system by training it to recognise 32 material types in both indoor and outdoor environments. Our approach produced recognition accuracies above 98% in 14,860 images of 15 indoor materials and above 89% in 26,584 images of 17 outdoor materials. We conclude by discussing its potentials for real-time use in HCI applications and future directions.
cs.CV cond-mat.mtrl-sci cs.HC cs.LG
we introduce deep thermal imaging a new approach for closerange automatic recognition of materials to enhance the understanding of people and ubiquitous technologies of their proximal environment our approach uses a lowcost mobile thermal camera integrated into a smartphone to capture thermal textures a deep neural network classifies these textures into material types this approach works effectively without the need for ambient light sources or direct contact with materials furthermore the use of a deep learning network removes the need to handcraft the set of features for different materials we evaluated the performance of the system by training it to recognise 32 material types in both indoor and outdoor environments our approach produced recognition accuracies above 98 in 14860 images of 15 indoor materials and above 89 in 26584 images of 17 outdoor materials we conclude by discussing its potentials for realtime use in hci applications and future directions
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1,803.02311
Ground-State Magnetization in Mixtures of a Few Ultra-Cold Fermions in One-Dimensional Traps
Ground-state properties of a few spin-$1/2$ ultra-cold fermions confined in a one-dimensional trap are studied by the exact diagonalization method. In contrast to previous studies, it is not assumed that the projection of a spin of individual particles is fixed. Therefore, the spin is treated as an additional degree of freedom and the global magnetization of the system is established spontaneously. Depending on the shape of the trap, inter-particle interactions, and an external magnetic field, the phase diagram of the system is determined. It is shown that, for particular confinements, some values of the magnetization cannot be reached by the ground-state of the system.
cond-mat.quant-gas
groundstate properties of a few spin12 ultracold fermions confined in a onedimensional trap are studied by the exact diagonalization method in contrast to previous studies it is not assumed that the projection of a spin of individual particles is fixed therefore the spin is treated as an additional degree of freedom and the global magnetization of the system is established spontaneously depending on the shape of the trap interparticle interactions and an external magnetic field the phase diagram of the system is determined it is shown that for particular confinements some values of the magnetization cannot be reached by the groundstate of the system
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1,803.02312
Dimensionality Reduction for Stationary Time Series via Stochastic Nonconvex Optimization
Stochastic optimization naturally arises in machine learning. Efficient algorithms with provable guarantees, however, are still largely missing, when the objective function is nonconvex and the data points are dependent. This paper studies this fundamental challenge through a streaming PCA problem for stationary time series data. Specifically, our goal is to estimate the principle component of time series data with respect to the covariance matrix of the stationary distribution. Computationally, we propose a variant of Oja's algorithm combined with downsampling to control the bias of the stochastic gradient caused by the data dependency. Theoretically, we quantify the uncertainty of our proposed stochastic algorithm based on diffusion approximations. This allows us to prove the asymptotic rate of convergence and further implies near optimal asymptotic sample complexity. Numerical experiments are provided to support our analysis.
cs.LG math.OC stat.ML
stochastic optimization naturally arises in machine learning efficient algorithms with provable guarantees however are still largely missing when the objective function is nonconvex and the data points are dependent this paper studies this fundamental challenge through a streaming pca problem for stationary time series data specifically our goal is to estimate the principle component of time series data with respect to the covariance matrix of the stationary distribution computationally we propose a variant of ojas algorithm combined with downsampling to control the bias of the stochastic gradient caused by the data dependency theoretically we quantify the uncertainty of our proposed stochastic algorithm based on diffusion approximations this allows us to prove the asymptotic rate of convergence and further implies near optimal asymptotic sample complexity numerical experiments are provided to support our analysis
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1,803.02313
Methods for separation of deuterons produced in the medium and in jets in high energy collisions
Coalescence has long been used to describe the production of light (anti-)nuclei in heavy ion collisions. The same underlying mechanism may also exist in jets when a proton and a neutron are close enough in phase space to form a deuteron. We model deuteron production in jets by applying an afterburner to protons and neutrons produced in PYTHIA for $p$+$p$ collisions at a center of mass energy $\sqrt{s} =$ 7 TeV. PYTHIA provides a reasonable description of the proton spectra and the shape of the deuteron spectrum predicted by the afterburner is in agreement with the data. We show that the rise in the coalescence parameter $B_2$ with momentum observed in data is consistent with coalescence in jets. We show that di-hadron correlations can be used to separate the contributions from the jet and the underlying event. This model predicts that the conditional coalescence parameter in the jet-like correlation should be independent of the trigger momentum.
hep-ph nucl-th
coalescence has long been used to describe the production of light antinuclei in heavy ion collisions the same underlying mechanism may also exist in jets when a proton and a neutron are close enough in phase space to form a deuteron we model deuteron production in jets by applying an afterburner to protons and neutrons produced in pythia for pp collisions at a center of mass energy sqrts 7 tev pythia provides a reasonable description of the proton spectra and the shape of the deuteron spectrum predicted by the afterburner is in agreement with the data we show that the rise in the coalescence parameter b_2 with momentum observed in data is consistent with coalescence in jets we show that dihadron correlations can be used to separate the contributions from the jet and the underlying event this model predicts that the conditional coalescence parameter in the jetlike correlation should be independent of the trigger momentum
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1,803.02314
The generalised Baker--Schmidt problem on hypersurfaces
The Generalised Baker--Schmidt Problem (1970) concerns the $f$-dimensional Hausdorff measure of the set of $\psi$-approximable points on a nondegenerate manifold. There are two variants of this problem, concerning simultaneous and dual approximation. Beresnevich--Dickinson--Velani (in 2006, for the homogeneous setting) and Badziahin--Beresnevich--Velani (in 2013, for the inhomogeneous setting) proved the divergence part of this problem for dual approximation on arbitrary nondegenerate manifolds. The corresponding convergence counterpart represents a major challenging open question and the progress thus far has only been attained over planar curves. In this paper, we settle this problem for hypersurfaces in a more general setting, i.e. for inhomogeneous approximations and with a non-monotonic multivariable approximating function.
math.NT
the generalised bakerschmidt problem 1970 concerns the fdimensional hausdorff measure of the set of psiapproximable points on a nondegenerate manifold there are two variants of this problem concerning simultaneous and dual approximation beresnevichdickinsonvelani in 2006 for the homogeneous setting and badziahinberesnevichvelani in 2013 for the inhomogeneous setting proved the divergence part of this problem for dual approximation on arbitrary nondegenerate manifolds the corresponding convergence counterpart represents a major challenging open question and the progress thus far has only been attained over planar curves in this paper we settle this problem for hypersurfaces in a more general setting ie for inhomogeneous approximations and with a nonmonotonic multivariable approximating function
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1,803.02315
Comparison of Deep Learning Approaches for Multi-Label Chest X-Ray Classification
The increased availability of X-ray image archives (e.g. the ChestX-ray14 dataset from the NIH Clinical Center) has triggered a growing interest in deep learning techniques. To provide better insight into the different approaches, and their applications to chest X-ray classification, we investigate a powerful network architecture in detail: the ResNet-50. Building on prior work in this domain, we consider transfer learning with and without fine-tuning as well as the training of a dedicated X-ray network from scratch. To leverage the high spatial resolution of X-ray data, we also include an extended ResNet-50 architecture, and a network integrating non-image data (patient age, gender and acquisition type) in the classification process. In a concluding experiment, we also investigate multiple ResNet depths (i.e. ResNet-38 and ResNet-101). In a systematic evaluation, using 5-fold re-sampling and a multi-label loss function, we compare the performance of the different approaches for pathology classification by ROC statistics and analyze differences between the classifiers using rank correlation. Overall, we observe a considerable spread in the achieved performance and conclude that the X-ray-specific ResNet-38, integrating non-image data yields the best overall results. Furthermore, class activation maps are used to understand the classification process, and a detailed analysis of the impact of non-image features is provided.
cs.CV
the increased availability of xray image archives eg the chestxray14 dataset from the nih clinical center has triggered a growing interest in deep learning techniques to provide better insight into the different approaches and their applications to chest xray classification we investigate a powerful network architecture in detail the resnet50 building on prior work in this domain we consider transfer learning with and without finetuning as well as the training of a dedicated xray network from scratch to leverage the high spatial resolution of xray data we also include an extended resnet50 architecture and a network integrating nonimage data patient age gender and acquisition type in the classification process in a concluding experiment we also investigate multiple resnet depths ie resnet38 and resnet101 in a systematic evaluation using 5fold resampling and a multilabel loss function we compare the performance of the different approaches for pathology classification by roc statistics and analyze differences between the classifiers using rank correlation overall we observe a considerable spread in the achieved performance and conclude that the xrayspecific resnet38 integrating nonimage data yields the best overall results furthermore class activation maps are used to understand the classification process and a detailed analysis of the impact of nonimage features is provided
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1,803.02316
Precision Light Curves from TESS Full-Frame Images: A Difference Imaging Approach
The Transiting Exoplanet Survey Satellite (TESS) will observe $\sim$150~million stars brighter than $T_{\rm mag} \approx 16$, with photometric precision from 60~ppm to 3~percent, enabling an array of exoplanet and stellar astrophysics investigations.While light curves will be provided for $\sim$400,000 targets observed at 2-min cadence, observations of most stars will only be provided as full-frame images (FFIs) at 30~min cadence. The TESS image scale of $\sim21$''/pix is highly susceptible to crowding, blending, and source confusion, and the highly spatially variable point spread function (PSF) will challenge traditional techniques, such as aperture and Gaussian-kernel PSF photometry. We use official "End-to-End~6" TESS simulated FFIs to demonstrate a difference image analysis pipeline, using a $\delta$-function kernel,that achieves the mission specification noise floor of 60~ppm~hr$^{-1/2}$. We show that the pipeline performance does not depend on position across the field, and only $\sim$2\% of stars appear to exhibit residual systematics at the level of $\sim$5~ppt. We also demonstrate recoverability of planet transits, eclipsing binaries, and other variables. We provide the pipeline as an open-source tool at https://github.com/ryanoelkers/DIA in both IDL and PYTHON. We intend to extract light curves for all point sources in the \textit{TESS} FFIs as soon as they become publicly available, and will provide the light curves through the Filtergraph data visualization service. An example data portal based on the simulated FFIs is available for inspection at https://filtergraph.com/tess_ffi.
astro-ph.IM
the transiting exoplanet survey satellite tess will observe sim150million stars brighter than t_rm mag approx 16 with photometric precision from 60ppm to 3percent enabling an array of exoplanet and stellar astrophysics investigationswhile light curves will be provided for sim400000 targets observed at 2min cadence observations of most stars will only be provided as fullframe images ffis at 30min cadence the tess image scale of sim21pix is highly susceptible to crowding blending and source confusion and the highly spatially variable point spread function psf will challenge traditional techniques such as aperture and gaussiankernel psf photometry we use official endtoend6 tess simulated ffis to demonstrate a difference image analysis pipeline using a deltafunction kernelthat achieves the mission specification noise floor of 60ppmhr12 we show that the pipeline performance does not depend on position across the field and only sim2 of stars appear to exhibit residual systematics at the level of sim5ppt we also demonstrate recoverability of planet transits eclipsing binaries and other variables we provide the pipeline as an opensource tool at httpsgithubcomryanoelkersdia in both idl and python we intend to extract light curves for all point sources in the textittess ffis as soon as they become publicly available and will provide the light curves through the filtergraph data visualization service an example data portal based on the simulated ffis is available for inspection at httpsfiltergraphcomtess_ffi
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1,803.02317
Conical Morris-Thorne Wormholes with a Global Monopole Charge
In this paper we have established an asymptotically conical Morris-Thorne wormhole solution supported by anisotropic matter fluid and a global monopole charge in the framework of a $1+3$ dimensional gravity minimally coupled to a triplet of scalar fields $\phi^a$, resulting from the breaking of a global $O(3)$ symmetry. For the anisotropic matter fluid we have considered the equation of state (EoS) given by $\mathcal{P}_r=\omega \rho$, with a consequence $\omega<-1$, implying a so-called phantom energy at the throat of the wormhole which violates the energy conditions. In addition, we study the weak gravitational lensing effect using the Gauss-Bonnet theorem (GBT) applied to the wormhole optical geometry. We show that the total deflection angle consists of a term given by $4\pi^2 \eta^2 $, which is independent from the impact parameter $b$, and an additional term which depends on the radius of the wormhole throat $b_0$ as well as the dimensionless constant $\zeta$.
gr-qc
in this paper we have established an asymptotically conical morristhorne wormhole solution supported by anisotropic matter fluid and a global monopole charge in the framework of a 13 dimensional gravity minimally coupled to a triplet of scalar fields phia resulting from the breaking of a global o3 symmetry for the anisotropic matter fluid we have considered the equation of state eos given by mathcalp_romega rho with a consequence omega1 implying a socalled phantom energy at the throat of the wormhole which violates the energy conditions in addition we study the weak gravitational lensing effect using the gaussbonnet theorem gbt applied to the wormhole optical geometry we show that the total deflection angle consists of a term given by 4pi2 eta2 which is independent from the impact parameter b and an additional term which depends on the radius of the wormhole throat b_0 as well as the dimensionless constant zeta
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1,803.02318
Stability of the Broad Line Region Geometry and Dynamics in Arp 151 Over Seven Years
The Seyfert 1 galaxy Arp 151 was monitored as part of three reverberation mapping campaigns spanning $2008-2015$. We present modeling of these velocity-resolved reverberation mapping datasets using a geometric and dynamical model for the broad line region (BLR). By modeling each of the three datasets independently, we infer the evolution of the BLR structure in Arp 151 over a total of seven years and constrain the systematic uncertainties in non-varying parameters such as the black hole mass. We find that the BLR geometry of a thick disk viewed close to face-on is stable over this time, although the size of the BLR grows by a factor of $\sim 2$. The dynamics of the BLR are dominated by inflow and the inferred black hole mass is consistent for the three datasets, despite the increase in BLR size. Combining the inference for the three datasets yields a black hole mass and statistical uncertainty of $\log_{10}($M$_{\rm BH}/\rm{M}_{\odot})=6.82^{+0.09}_{-0.09}$ with a standard deviation in individual measurements of 0.13 dex.
astro-ph.GA
the seyfert 1 galaxy arp 151 was monitored as part of three reverberation mapping campaigns spanning 20082015 we present modeling of these velocityresolved reverberation mapping datasets using a geometric and dynamical model for the broad line region blr by modeling each of the three datasets independently we infer the evolution of the blr structure in arp 151 over a total of seven years and constrain the systematic uncertainties in nonvarying parameters such as the black hole mass we find that the blr geometry of a thick disk viewed close to faceon is stable over this time although the size of the blr grows by a factor of sim 2 the dynamics of the blr are dominated by inflow and the inferred black hole mass is consistent for the three datasets despite the increase in blr size combining the inference for the three datasets yields a black hole mass and statistical uncertainty of log_10m_rm bhrmm_odot682009_009 with a standard deviation in individual measurements of 013 dex
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1,803.02319
Upper Covers of Chains and Antichains in Sets of Indecomposable Subsets
We prove that there are arbitrarily large indecomposable ordered sets T with a 2-chain C such that the smallest indecomposable proper superset U of C in T is T itself. Subsequently, we characterize all such indecomposable ordered sets T and 2-chains C. We also prove the same type of result for 2-antichains.
math.CO
we prove that there are arbitrarily large indecomposable ordered sets t with a 2chain c such that the smallest indecomposable proper superset u of c in t is t itself subsequently we characterize all such indecomposable ordered sets t and 2chains c we also prove the same type of result for 2antichains
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1,803.0232
Argyres-Douglas theories, Painlev\'e II and quantum mechanics
We show in details that the all-orders genus expansion of the two-cut Hermitian cubic matrix model reproduces the perturbative expansion of the $H_1$ Argyres-Douglas theory coupled to the $\Omega$ background. In the self-dual limit we use the Painlev\'e/gauge correspondence and we show that, after summing over all instanton sectors, the two-cut cubic matrix model computes the tau function of Painlev\'e II without taking any double scaling limit or adding any external fields. We decode such solution within the context of trans-series. Finally in the Nekrasov-Shatashvili limit we connect the $H_1$ and the $H_0$ Argyres-Douglas theories to the quantum mechanical models with cubic and double well potentials.
hep-th math-ph math.MP
we show in details that the allorders genus expansion of the twocut hermitian cubic matrix model reproduces the perturbative expansion of the h_1 argyresdouglas theory coupled to the omega background in the selfdual limit we use the painlevegauge correspondence and we show that after summing over all instanton sectors the twocut cubic matrix model computes the tau function of painleve ii without taking any double scaling limit or adding any external fields we decode such solution within the context of transseries finally in the nekrasovshatashvili limit we connect the h_1 and the h_0 argyresdouglas theories to the quantum mechanical models with cubic and double well potentials
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1,803.02321
Monte Carlo Top Quark Mass Calibration
The most precise top quark mass measurements use kinematic reconstruction methods, determining the top mass parameter of a Monte Carlo event generator, $m_t^{\rm MC}$. Due to the complicated interplay of hadronization and parton shower dynamics in Monte Carlo event generators relevant for kinematic reconstruction, relating $m_t^{\rm MC}$ to field theory masses is a non-trivial task. In this talk we report on a calibration procedure to determine this relation using hadron level QCD predictions for 2-Jettiness in $e^+e^-$ annihilation, an observable which has kinematic top mass sensitivity and a close relation to the invariant mass of the particles coming from the top decay. The theoretical ingredients of the QCD prediction are reviewed. Fitting $e^+e^-$ 2-Jettiness calculations at NLL/NNLL order to PYTHIA 8.205, we find that $m_t^{\rm MC}$ agrees with the MSR mass $m_{t,1\,{\rm GeV}}^{\rm MSR}$ within uncertainties. At NNLL we find $m_t^{\rm MC} = m_{t,1\,{\rm GeV}}^{\rm MSR} + (0.18 \pm 0.22)\,{\rm GeV}$. $m_t^{\rm MC}$ can differ from the pole mass $m_t^{\rm pole}$ by up to $600\,{\rm MeV}$, and using the pole mass generally leads to larger uncertainties. At NNLL we find $m_t^{\rm MC} = m_t^{\rm pole} + (0.57 \pm 0.28)\,{\rm GeV}$ as the fit result. In contrast, converting $m_{t,1\,{\rm GeV}}^{\rm MSR}$ obtained at NNLL to the pole mass gives a result for $m_t^{\rm pole}$ that is substantially larger and incompatible with the fit result. We also explain some theoretical aspects relevant for employing the C-parameter as an alternative calibration observable.
hep-ph
the most precise top quark mass measurements use kinematic reconstruction methods determining the top mass parameter of a monte carlo event generator m_trm mc due to the complicated interplay of hadronization and parton shower dynamics in monte carlo event generators relevant for kinematic reconstruction relating m_trm mc to field theory masses is a nontrivial task in this talk we report on a calibration procedure to determine this relation using hadron level qcd predictions for 2jettiness in ee annihilation an observable which has kinematic top mass sensitivity and a close relation to the invariant mass of the particles coming from the top decay the theoretical ingredients of the qcd prediction are reviewed fitting ee 2jettiness calculations at nllnnll order to pythia 8205 we find that m_trm mc agrees with the msr mass m_t1rm gevrm msr within uncertainties at nnll we find m_trm mc m_t1rm gevrm msr 018 pm 022rm gev m_trm mc can differ from the pole mass m_trm pole by up to 600rm mev and using the pole mass generally leads to larger uncertainties at nnll we find m_trm mc m_trm pole 057 pm 028rm gev as the fit result in contrast converting m_t1rm gevrm msr obtained at nnll to the pole mass gives a result for m_trm pole that is substantially larger and incompatible with the fit result we also explain some theoretical aspects relevant for employing the cparameter as an alternative calibration observable
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1,803.02322
Singular quasisymmetric mappings in dimensions two and greater
For all $n \geq 2$, we construct a metric space $(X,d)$ and a quasisymmetric mapping $f\colon [0,1]^n \rightarrow X$ with the property that $f^{-1}$ is not absolutely continuous with respect to the Hausdorff $n$-measure on $X$. That is, there exists a Borel set $E \subset [0,1]^n$ with Lebesgue measure $|E|>0$ such that $f(E)$ has Hausdorff $n$-measure zero. The construction may be carried out so that $X$ has finite Hausdorff $n$-measure and $|E|$ is arbitrarily close to 1, or so that $|E| = 1$. This gives a negative answer to a question of Heinonen and Semmes.
math.MG
for all n geq 2 we construct a metric space xd and a quasisymmetric mapping fcolon 01n rightarrow x with the property that f1 is not absolutely continuous with respect to the hausdorff nmeasure on x that is there exists a borel set e subset 01n with lebesgue measure e0 such that fe has hausdorff nmeasure zero the construction may be carried out so that x has finite hausdorff nmeasure and e is arbitrarily close to 1 or so that e 1 this gives a negative answer to a question of heinonen and semmes
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1,803.02323
Deep Super Learner: A Deep Ensemble for Classification Problems
Deep learning has become very popular for tasks such as predictive modeling and pattern recognition in handling big data. Deep learning is a powerful machine learning method that extracts lower level features and feeds them forward for the next layer to identify higher level features that improve performance. However, deep neural networks have drawbacks, which include many hyper-parameters and infinite architectures, opaqueness into results, and relatively slower convergence on smaller datasets. While traditional machine learning algorithms can address these drawbacks, they are not typically capable of the performance levels achieved by deep neural networks. To improve performance, ensemble methods are used to combine multiple base learners. Super learning is an ensemble that finds the optimal combination of diverse learning algorithms. This paper proposes deep super learning as an approach which achieves log loss and accuracy results competitive to deep neural networks while employing traditional machine learning algorithms in a hierarchical structure. The deep super learner is flexible, adaptable, and easy to train with good performance across different tasks using identical hyper-parameter values. Using traditional machine learning requires fewer hyper-parameters, allows transparency into results, and has relatively fast convergence on smaller datasets. Experimental results show that the deep super learner has superior performance compared to the individual base learners, single-layer ensembles, and in some cases deep neural networks. Performance of the deep super learner may further be improved with task-specific tuning.
cs.LG stat.ML
deep learning has become very popular for tasks such as predictive modeling and pattern recognition in handling big data deep learning is a powerful machine learning method that extracts lower level features and feeds them forward for the next layer to identify higher level features that improve performance however deep neural networks have drawbacks which include many hyperparameters and infinite architectures opaqueness into results and relatively slower convergence on smaller datasets while traditional machine learning algorithms can address these drawbacks they are not typically capable of the performance levels achieved by deep neural networks to improve performance ensemble methods are used to combine multiple base learners super learning is an ensemble that finds the optimal combination of diverse learning algorithms this paper proposes deep super learning as an approach which achieves log loss and accuracy results competitive to deep neural networks while employing traditional machine learning algorithms in a hierarchical structure the deep super learner is flexible adaptable and easy to train with good performance across different tasks using identical hyperparameter values using traditional machine learning requires fewer hyperparameters allows transparency into results and has relatively fast convergence on smaller datasets experimental results show that the deep super learner has superior performance compared to the individual base learners singlelayer ensembles and in some cases deep neural networks performance of the deep super learner may further be improved with taskspecific tuning
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1,803.02324
Annotation Artifacts in Natural Language Inference Data
Large-scale datasets for natural language inference are created by presenting crowd workers with a sentence (premise), and asking them to generate three new sentences (hypotheses) that it entails, contradicts, or is logically neutral with respect to. We show that, in a significant portion of such data, this protocol leaves clues that make it possible to identify the label by looking only at the hypothesis, without observing the premise. Specifically, we show that a simple text categorization model can correctly classify the hypothesis alone in about 67% of SNLI (Bowman et. al, 2015) and 53% of MultiNLI (Williams et. al, 2017). Our analysis reveals that specific linguistic phenomena such as negation and vagueness are highly correlated with certain inference classes. Our findings suggest that the success of natural language inference models to date has been overestimated, and that the task remains a hard open problem.
cs.CL cs.AI
largescale datasets for natural language inference are created by presenting crowd workers with a sentence premise and asking them to generate three new sentences hypotheses that it entails contradicts or is logically neutral with respect to we show that in a significant portion of such data this protocol leaves clues that make it possible to identify the label by looking only at the hypothesis without observing the premise specifically we show that a simple text categorization model can correctly classify the hypothesis alone in about 67 of snli bowman et al 2015 and 53 of multinli williams et al 2017 our analysis reveals that specific linguistic phenomena such as negation and vagueness are highly correlated with certain inference classes our findings suggest that the success of natural language inference models to date has been overestimated and that the task remains a hard open problem
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1,803.02325
Light Ion Accelerating Line (L3IA): Test Experiment at ILIL-PW
The construction of a novel Laser driven Light Ions Acceleration Line(L3IA) is progressing rapidly towards the operation, following the recent upgrade of the ILIL-PW laser facility. The Line was designed following the pilot experimental activity carried out earlier at the same facility to define design parameters and to identify main components including target control and diagnostic equipment, also in combination with the numerical simulations for the optimization of laser and target parameters. A preliminary set of data was acquired following the successful commissioning of the laser system >100 TW upgrade. Data include output from a range of different ion detectors and optical diagnostics installed for qualification of the laser-target interaction. An overview of the results is given along with a description of the relevant upgraded laser facility and features.
physics.plasm-ph
the construction of a novel laser driven light ions acceleration linel3ia is progressing rapidly towards the operation following the recent upgrade of the ililpw laser facility the line was designed following the pilot experimental activity carried out earlier at the same facility to define design parameters and to identify main components including target control and diagnostic equipment also in combination with the numerical simulations for the optimization of laser and target parameters a preliminary set of data was acquired following the successful commissioning of the laser system 100 tw upgrade data include output from a range of different ion detectors and optical diagnostics installed for qualification of the lasertarget interaction an overview of the results is given along with a description of the relevant upgraded laser facility and features
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1,803.02326
Comparison of various image fusion methods for impervious surface classification from VNREDSat-1
Impervious surface is an important indicator for urban development monitoring. Accurate urban impervious surfaces mapping with VNREDSat-1 remains challenging due to their spectral diversity not captured by individual PAN image. In this artical, five multi-resolution image fusion techniques were compared for classification task of urban impervious surface. The result shows that for VNREDSat-1 dataset, UNB and Wavelet tranform methods are the best techniques reserving spatial and spectral information of original MS image, respectively. However, the UNB technique gives best results when it comes to impervious surface classification especially in the case of shadow area included in non-impervious surface group.
cs.CV
impervious surface is an important indicator for urban development monitoring accurate urban impervious surfaces mapping with vnredsat1 remains challenging due to their spectral diversity not captured by individual pan image in this artical five multiresolution image fusion techniques were compared for classification task of urban impervious surface the result shows that for vnredsat1 dataset unb and wavelet tranform methods are the best techniques reserving spatial and spectral information of original ms image respectively however the unb technique gives best results when it comes to impervious surface classification especially in the case of shadow area included in nonimpervious surface group
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1,803.02327
On the stationary solutions of Doi-Onsager model in general dimension
We give new results of the phase transition of dilute colloidal solutions of rod-like molecules in dimension $D \geq 3$. For the low concentration of particles in a carrier fluid, we prove that the isotropic phase is the unique solution to the Doi-Onsager model with the general potential kernel. In addition, we present the regime of the bifurcation of nematic phases in the class of axially symmetric solutions. Our method is based on a generalization of the classical Leray-Schauder degree we developed for this problem.
math.AP
we give new results of the phase transition of dilute colloidal solutions of rodlike molecules in dimension d geq 3 for the low concentration of particles in a carrier fluid we prove that the isotropic phase is the unique solution to the doionsager model with the general potential kernel in addition we present the regime of the bifurcation of nematic phases in the class of axially symmetric solutions our method is based on a generalization of the classical lerayschauder degree we developed for this problem
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1,803.02328
Hidden Symmetries in Real and Theoretical Networks
Symmetries are ubiquitous in real networks and often characterize network features and functions. Here we present a generalization of network symmetry called \emph{latent symmetry}, which is an extension of the standard notion of symmetry. They are defined in terms of standard symmetries in a reduced version of the network. One unique aspect of latent symmetries is that each one is associated with a \emph{size}, which provides a way of discussing symmetries at multiple scales in a network. We are able to demonstrate a number of examples of networks (graphs) which contain latent symmetry, including a number of real networks. In numerical experiments, we show that latent symmetries are found more frequently in graphs built using preferential attachment, a standard model of network growth, when compared to non-network like (Erd{\H o}s-R\'enyi) graphs. Finally we prove that if vertices in a network are latently symmetric, then they must have the same eigenvector centrality, similar to vertices which are symmetric in the standard sense. This suggests that the latent symmetries present in real-networks may serve the same structural and functional purpose standard symmetries do in these networks. We conclude from these facts and observations that \emph{latent symmetries} are present in real networks and provide useful information about the network potentially beyond standard symmetries as they can appear at multiple scales.
physics.soc-ph cond-mat.dis-nn cs.SI
symmetries are ubiquitous in real networks and often characterize network features and functions here we present a generalization of network symmetry called emphlatent symmetry which is an extension of the standard notion of symmetry they are defined in terms of standard symmetries in a reduced version of the network one unique aspect of latent symmetries is that each one is associated with a emphsize which provides a way of discussing symmetries at multiple scales in a network we are able to demonstrate a number of examples of networks graphs which contain latent symmetry including a number of real networks in numerical experiments we show that latent symmetries are found more frequently in graphs built using preferential attachment a standard model of network growth when compared to nonnetwork like erdh osrenyi graphs finally we prove that if vertices in a network are latently symmetric then they must have the same eigenvector centrality similar to vertices which are symmetric in the standard sense this suggests that the latent symmetries present in realnetworks may serve the same structural and functional purpose standard symmetries do in these networks we conclude from these facts and observations that emphlatent symmetries are present in real networks and provide useful information about the network potentially beyond standard symmetries as they can appear at multiple scales
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1,803.02329
Learning Memory Access Patterns
The explosion in workload complexity and the recent slow-down in Moore's law scaling call for new approaches towards efficient computing. Researchers are now beginning to use recent advances in machine learning in software optimizations, augmenting or replacing traditional heuristics and data structures. However, the space of machine learning for computer hardware architecture is only lightly explored. In this paper, we demonstrate the potential of deep learning to address the von Neumann bottleneck of memory performance. We focus on the critical problem of learning memory access patterns, with the goal of constructing accurate and efficient memory prefetchers. We relate contemporary prefetching strategies to n-gram models in natural language processing, and show how recurrent neural networks can serve as a drop-in replacement. On a suite of challenging benchmark datasets, we find that neural networks consistently demonstrate superior performance in terms of precision and recall. This work represents the first step towards practical neural-network based prefetching, and opens a wide range of exciting directions for machine learning in computer architecture research.
cs.LG stat.ML
the explosion in workload complexity and the recent slowdown in moores law scaling call for new approaches towards efficient computing researchers are now beginning to use recent advances in machine learning in software optimizations augmenting or replacing traditional heuristics and data structures however the space of machine learning for computer hardware architecture is only lightly explored in this paper we demonstrate the potential of deep learning to address the von neumann bottleneck of memory performance we focus on the critical problem of learning memory access patterns with the goal of constructing accurate and efficient memory prefetchers we relate contemporary prefetching strategies to ngram models in natural language processing and show how recurrent neural networks can serve as a dropin replacement on a suite of challenging benchmark datasets we find that neural networks consistently demonstrate superior performance in terms of precision and recall this work represents the first step towards practical neuralnetwork based prefetching and opens a wide range of exciting directions for machine learning in computer architecture research
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1,803.0233
On almost revlex ideals with Hilbert function of complete intersections
In this paper, we investigate the behavior of almost reverse lexicographic ideals with the Hilbert function of a complete intersection. More precisely, over a field $K$, we give a new constructive proof of the existence of the almost revlex ideal $J\subset K[x_1,\dots,x_n]$, with the same Hilbert function as a complete intersection defined by $n$ forms of degrees $d_1\leq \dots \leq d_n$. Properties of the reduction numbers for an almost revlex ideal have an important role in our inductive and constructive proof, which is different from the more general construction given by Pardue in 2010. We also detect several cases in which an almost revlex ideal having the same Hilbert function as a complete intersection corresponds to a singular point in a Hilbert scheme. This second result is the outcome of a more general study of lower bounds for the dimension of the tangent space to a Hilbert scheme at stable ideals, in terms of the number of minimal generators.
math.AC
in this paper we investigate the behavior of almost reverse lexicographic ideals with the hilbert function of a complete intersection more precisely over a field k we give a new constructive proof of the existence of the almost revlex ideal jsubset kx_1dotsx_n with the same hilbert function as a complete intersection defined by n forms of degrees d_1leq dots leq d_n properties of the reduction numbers for an almost revlex ideal have an important role in our inductive and constructive proof which is different from the more general construction given by pardue in 2010 we also detect several cases in which an almost revlex ideal having the same hilbert function as a complete intersection corresponds to a singular point in a hilbert scheme this second result is the outcome of a more general study of lower bounds for the dimension of the tangent space to a hilbert scheme at stable ideals in terms of the number of minimal generators
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1,803.02331
Pathways to Fragmentation:User Flows and Web Distribution Infrastructures
This study analyzes how web audiences flow across online digital features. We construct a directed network of user flows based on sequential user clickstreams for all popular websites (n=1761), using traffic data obtained from a panel of a million web users in the United States. We analyze these data to identify constellations of websites that are frequently browsed together in temporal sequences, both by similar user groups in different browsing sessions as well as by disparate users. Our analyses thus render visible previously hidden online collectives and generate insight into the varied roles that curatorial infrastructures may play in shaping audience fragmentation on the web.
cs.CY
this study analyzes how web audiences flow across online digital features we construct a directed network of user flows based on sequential user clickstreams for all popular websites n1761 using traffic data obtained from a panel of a million web users in the united states we analyze these data to identify constellations of websites that are frequently browsed together in temporal sequences both by similar user groups in different browsing sessions as well as by disparate users our analyses thus render visible previously hidden online collectives and generate insight into the varied roles that curatorial infrastructures may play in shaping audience fragmentation on the web
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1,803.02332
The Frankel property for self-shrinkers from the viewpoint of elliptic PDE's
We show that two properly embedded self-shrinkers in Euclidean space that are sufficiently separated at infinity must intersect at a finite point. The proof is based on a localized version of the Reilly formula applied to a suitable f-harmonic function with controlled gradient. In the immersed case, a new direct proof of the generalized half-space property is also presented.
math.DG
we show that two properly embedded selfshrinkers in euclidean space that are sufficiently separated at infinity must intersect at a finite point the proof is based on a localized version of the reilly formula applied to a suitable fharmonic function with controlled gradient in the immersed case a new direct proof of the generalized halfspace property is also presented
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1,803.02333
Eilenberg--Mac Lane Spaces for Topological Groups
The goal of this paper is to establish a topological version of the notion of an Eilenberg-Mac Lane space. If $X$ is a pointed topological space, $\pi_1(X)$ has a natural topology coming from the compact-open topology on the space of maps $S^1 \to X$. In general the construction does not produce a topological group because it is possible to create examples where the group multiplication $\pi_1(X) \times \pi_1(X) \to \pi_1(X)$ is discontinuous. This failure to obtain a topological group has been noticed by others, for example Fabel. However, if we work in the category of compactly generated, weakly Hausdorff spaces, we may retopologise both the space of maps $S^1 \to X$ and the product $\pi_1(X) \times \pi_1(X)$ with compactly generated topologies to get that $\pi_1(X)$ is a group object in this category. Such group objects are known as $k$-groups. Next we construct the Eilenberg-Mac Lane space $K(G,1)$ for any totally path-disconnected $k$-group $G$. The main point of this paper is to show that, for such a $G$, $\pi_1(K(G,1))$ is isomorphic to $G$ in the category of $k$-groups. All totally disconnected locally compact groups are $k$-groups and so our results apply in particular to profinite groups. This answers questions that have been raised by Sauer. We also show that there are Mayer-Vietoris sequences and a Seifert-van Kampen theorem in this theory. The theory requires a careful analysis using model structures and other homotopical structures on cartesian closed categories as we shall see that no theory can be comfortably developed in the classical world.
math.GR math.AT
the goal of this paper is to establish a topological version of the notion of an eilenbergmac lane space if x is a pointed topological space pi_1x has a natural topology coming from the compactopen topology on the space of maps s1 to x in general the construction does not produce a topological group because it is possible to create examples where the group multiplication pi_1x times pi_1x to pi_1x is discontinuous this failure to obtain a topological group has been noticed by others for example fabel however if we work in the category of compactly generated weakly hausdorff spaces we may retopologise both the space of maps s1 to x and the product pi_1x times pi_1x with compactly generated topologies to get that pi_1x is a group object in this category such group objects are known as kgroups next we construct the eilenbergmac lane space kg1 for any totally pathdisconnected kgroup g the main point of this paper is to show that for such a g pi_1kg1 is isomorphic to g in the category of kgroups all totally disconnected locally compact groups are kgroups and so our results apply in particular to profinite groups this answers questions that have been raised by sauer we also show that there are mayervietoris sequences and a seifertvan kampen theorem in this theory the theory requires a careful analysis using model structures and other homotopical structures on cartesian closed categories as we shall see that no theory can be comfortably developed in the classical world
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1,803.02334
A Nonparametric Approach to Measure the Heterogeneous Spatial Association: Under Spatial Temporal Data
Spatial association and heterogeneity are two critical areas in the research about spatial analysis, geography, statistics and so on. Though large amounts of outstanding methods has been proposed and studied, there are few of them tend to study spatial association under heterogeneous environment. Additionally, most of the traditional methods are based on distance statistic and spatial weighted matrix. However, in some abstract spatial situations, distance statistic can not be applied since we can not even observe the geographical locations directly. Meanwhile, under these circumstances, due to invisibility of spatial positions, designing of weight matrix can not absolutely avoid subjectivity. In this paper, a new entropy-based method, which is data-driven and distribution-free, has been proposed to help us investigate spatial association while fully taking the fact that heterogeneity widely exist. Specifically, this method is not bounded with distance statistic or weight matrix. Asymmetrical dependence is adopted to reflect the heterogeneity in spatial association for each individual and the whole discussion in this paper is performed on spatio-temporal data with only assuming stationary m-dependent over time.
econ.EM
spatial association and heterogeneity are two critical areas in the research about spatial analysis geography statistics and so on though large amounts of outstanding methods has been proposed and studied there are few of them tend to study spatial association under heterogeneous environment additionally most of the traditional methods are based on distance statistic and spatial weighted matrix however in some abstract spatial situations distance statistic can not be applied since we can not even observe the geographical locations directly meanwhile under these circumstances due to invisibility of spatial positions designing of weight matrix can not absolutely avoid subjectivity in this paper a new entropybased method which is datadriven and distributionfree has been proposed to help us investigate spatial association while fully taking the fact that heterogeneity widely exist specifically this method is not bounded with distance statistic or weight matrix asymmetrical dependence is adopted to reflect the heterogeneity in spatial association for each individual and the whole discussion in this paper is performed on spatiotemporal data with only assuming stationary mdependent over time
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1,803.02335
Mass generation and deconfinement in pure Yang-Mills theory: a variational study
A simple variational argument based on the Gaussian Effective Potential (GEP) is put forward to give evidence for mass generation and deconfinement in pure Yang-Mills SU(N) theory. The GEP analysis shows that the massless gaussian vacuum of Yang-Mills theory is perturbatively unstable towards a massive gaussian vacuum, indicating that a massive expansion is the natural choice for computations in YMT. At finite temperature, the GEP provides an optimal temperature-dependent mass parameter for the expansion and signals the occurrence of a weakly first-order phase transition at $T_{c}\approx$ 255 MeV for $N=3$. The equation of state is found to be in good agreement with the lattice data. This work is complemented with review material on the standard and massive expansions of Yang-Mills theory and on the formalism of quantum field theory at finite temperature. Comparisons are made with lattice results and numerical tables are provided to support our findings.
hep-th
a simple variational argument based on the gaussian effective potential gep is put forward to give evidence for mass generation and deconfinement in pure yangmills sun theory the gep analysis shows that the massless gaussian vacuum of yangmills theory is perturbatively unstable towards a massive gaussian vacuum indicating that a massive expansion is the natural choice for computations in ymt at finite temperature the gep provides an optimal temperaturedependent mass parameter for the expansion and signals the occurrence of a weakly firstorder phase transition at t_capprox 255 mev for n3 the equation of state is found to be in good agreement with the lattice data this work is complemented with review material on the standard and massive expansions of yangmills theory and on the formalism of quantum field theory at finite temperature comparisons are made with lattice results and numerical tables are provided to support our findings
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1,803.02336
A symmetric $\beta$-model
We prove that there exists a countable $\beta$-model in which, for all reals $X$ and $Y$, $X$ is definable from $Y$ if and only $X$ is hyperarithmetical in $Y$. We also obtain some related results and pose some related questions.
math.LO
we prove that there exists a countable betamodel in which for all reals x and y x is definable from y if and only x is hyperarithmetical in y we also obtain some related results and pose some related questions
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1,803.02337
Cyber-Physical Testbed for Power System Wide-Area Measurement-Based Control Using Open-Source Software
The electric power system is a cyber-physical system with power flow in the physical system and information flow in the cyber. Simulation is crucial to understanding the dynamics and control of electric power systems yet the underlying communication system has historically been ignored in these studies. This paper aims at meeting the increasing needs to simulate the operations of a real power system including the physical system, the energy management system, the communication system, and the emerging wide-area measurement-based controls. This paper proposes a cyber-physical testbed design and implementation for verifying and demonstrating wide-area control methods based on streaming telemetry and phasor measurement unit data. The proposed decoupled architecture is composed of a differential algebraic equation based physical system simulator, a software-defined network, a scripting language environment for prototyping an EMS system and a control system, all of which are integrated over industry-standard communication protocols. The proposed testbed is implemented using open-source software packages managed by a Python dispatcher. Finally, demonstrations are presented to show two wide-area measurement-based controls - system separation control and hierarchical voltage control, in the implemented testbed.
cs.SY cs.SE
the electric power system is a cyberphysical system with power flow in the physical system and information flow in the cyber simulation is crucial to understanding the dynamics and control of electric power systems yet the underlying communication system has historically been ignored in these studies this paper aims at meeting the increasing needs to simulate the operations of a real power system including the physical system the energy management system the communication system and the emerging widearea measurementbased controls this paper proposes a cyberphysical testbed design and implementation for verifying and demonstrating widearea control methods based on streaming telemetry and phasor measurement unit data the proposed decoupled architecture is composed of a differential algebraic equation based physical system simulator a softwaredefined network a scripting language environment for prototyping an ems system and a control system all of which are integrated over industrystandard communication protocols the proposed testbed is implemented using opensource software packages managed by a python dispatcher finally demonstrations are presented to show two widearea measurementbased controls system separation control and hierarchical voltage control in the implemented testbed
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1,803.02338
The CARMENES search for exoplanets around M dwarfs: Radial-velocity variations of active stars in visual-channel spectra
Previous simulations predicted the activity-induced radial-velocity (RV) variations of M dwarfs to range from $\sim1$ cm/s to $\sim1$ km/s, depending on various stellar and activity parameters. We investigate the observed relations between RVs, stellar activity, and stellar parameters of M dwarfs by analyzing CARMENES high-resolution visual-channel spectra ($0.5$$-$$1$$\mu$m), which were taken within the CARMENES RV planet survey during its first $20$ months of operation. During this time, $287$ of the CARMENES-sample stars were observed at least five times. From each spectrum we derived a relative RV and a measure of chromospheric H$\alpha$ emission. In addition, we estimated the chromatic index (CRX) of each spectrum, which is a measure of the RV wavelength dependence. Despite having a median number of only $11$ measurements per star, we show that the RV variations of the stars with RV scatter of $>10$ m/s and a projected rotation velocity $v \sin{i}>2$ km/s are caused mainly by activity. We name these stars `active RV-loud stars' and find their occurrence to increase with spectral type: from $\sim3\%$ for early-type M dwarfs (M$0.0$$-$$2.5$V) through $\sim30\%$ for mid-type M dwarfs (M$3.0$$-$$5.5$V) to $>50\%$ for late-type M dwarfs (M$6.0$$-$$9.0$V). Their RV-scatter amplitude is found to be correlated mainly with $v \sin{i}$. For about half of the stars, we also find a linear RV$-$CRX anticorrelation, which indicates that their activity-induced RV scatter is lower at longer wavelengths. For most of them we can exclude a linear correlation between RV and H$\alpha$ emission. Our results are in agreement with simulated activity-induced RV variations in M dwarfs. The RV variations of most active RV-loud M dwarfs are likely to be caused by dark spots on their surfaces, which move in and out of view as the stars rotate.
astro-ph.SR astro-ph.EP
previous simulations predicted the activityinduced radialvelocity rv variations of m dwarfs to range from sim1 cms to sim1 kms depending on various stellar and activity parameters we investigate the observed relations between rvs stellar activity and stellar parameters of m dwarfs by analyzing carmenes highresolution visualchannel spectra 051mum which were taken within the carmenes rv planet survey during its first 20 months of operation during this time 287 of the carmenessample stars were observed at least five times from each spectrum we derived a relative rv and a measure of chromospheric halpha emission in addition we estimated the chromatic index crx of each spectrum which is a measure of the rv wavelength dependence despite having a median number of only 11 measurements per star we show that the rv variations of the stars with rv scatter of 10 ms and a projected rotation velocity v sini2 kms are caused mainly by activity we name these stars active rvloud stars and find their occurrence to increase with spectral type from sim3 for earlytype m dwarfs m0025v through sim30 for midtype m dwarfs m3055v to 50 for latetype m dwarfs m6090v their rvscatter amplitude is found to be correlated mainly with v sini for about half of the stars we also find a linear rvcrx anticorrelation which indicates that their activityinduced rv scatter is lower at longer wavelengths for most of them we can exclude a linear correlation between rv and halpha emission our results are in agreement with simulated activityinduced rv variations in m dwarfs the rv variations of most active rvloud m dwarfs are likely to be caused by dark spots on their surfaces which move in and out of view as the stars rotate
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1,803.02339
Weakly trapped surfaces in asymptotically de Sitter spacetimes
It is a standard fact that trapped or marginally trapped surfaces are not visible from conformal infinity, under the usual set of conditions on matter fields and the conformal completion, provided that the cosmological constant is non-positive. In this note we show that the situation is more delicate in the presence of a positive cosmological constant: we present examples of visible marginally trapped surfaces, and we provide a set of natural conditions which guarantee non-visibility.
gr-qc
it is a standard fact that trapped or marginally trapped surfaces are not visible from conformal infinity under the usual set of conditions on matter fields and the conformal completion provided that the cosmological constant is nonpositive in this note we show that the situation is more delicate in the presence of a positive cosmological constant we present examples of visible marginally trapped surfaces and we provide a set of natural conditions which guarantee nonvisibility
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1,803.0234
A Window On The Earliest Star Formation: Extreme Photoionization Conditions of a High-Ionization, Low-Metallicity Lensed Galaxy at z~2
We report new observations of SL2SJ021737-051329, a lens system consisting of a bright arc at z=1.84435, magnified ~17x by a massive galaxy at z=0.65. SL2SJ0217 is a low-mass (M <10^9 M*), low-metallicity (Z~1/20 Z*) galaxy, with extreme star-forming conditions that produce strong nebular UV emission lines in the absence of any apparent outflows. Here we present several notable features from rest-frame UV Keck/LRIS spectroscopy: (1) Very strong narrow emission lines are measured for CIV 1548,1550, HeII 1640, OIII] 1661,1666, SiIII] 1883,1892, and CIII] 1907,1909. (2) Double-peaked LyA emission is observed with a dominant blue peak and centered near the systemic velocity. (3) The low- and high-ionization absorption features indicate very little or no outflowing gas along the sightline to the lensed galaxy. The relative emission line strengths can be reproduced with a very high-ionization, low-metallicity starburst with binaries, with the exception of He \ii, which indicates an additional ionization source is needed. We rule out large contributions from AGN and shocks to the photoionization budget, suggesting that the emission features requiring the hardest radiation field likely result from extreme stellar populations that are beyond the capabilities of current models. Therefore, SL2S0217 serves as a template for the extreme conditions that are important for reionization and thought to be more common in the early Universe.
astro-ph.GA
we report new observations of sl2sj021737051329 a lens system consisting of a bright arc at z184435 magnified 17x by a massive galaxy at z065 sl2sj0217 is a lowmass m 109 m lowmetallicity z120 z galaxy with extreme starforming conditions that produce strong nebular uv emission lines in the absence of any apparent outflows here we present several notable features from restframe uv kecklris spectroscopy 1 very strong narrow emission lines are measured for civ 15481550 heii 1640 oiii 16611666 siiii 18831892 and ciii 19071909 2 doublepeaked lya emission is observed with a dominant blue peak and centered near the systemic velocity 3 the low and highionization absorption features indicate very little or no outflowing gas along the sightline to the lensed galaxy the relative emission line strengths can be reproduced with a very highionization lowmetallicity starburst with binaries with the exception of he ii which indicates an additional ionization source is needed we rule out large contributions from agn and shocks to the photoionization budget suggesting that the emission features requiring the hardest radiation field likely result from extreme stellar populations that are beyond the capabilities of current models therefore sl2s0217 serves as a template for the extreme conditions that are important for reionization and thought to be more common in the early universe
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1,803.02341
Applications of Graded Methods to Cluster Variables in Arbitrary Types
This thesis is concerned with studying the properties of gradings on several examples of cluster algebras, primarily of infinite type. We first consider two finite type cases: $B_n$ and $C_n$, completing a classification by Grabowski for coefficient-free finite type cluster algebras. We then consider gradings arising from $3 \times 3$ skew-symmetric matrices. We show that the mutation-cyclic matrices give rise to gradings in which all degrees are positive and have only finitely many associated cluster variables (excepting one particular case). For the mutation-acyclic matrices, we prove that all occurring degrees have infinitely many variables. We provide a sufficient condition for a graded cluster algebra generated by a quiver to have infinitely many degrees, based on the presence of a subquiver in its mutation class. We use this to show that the cluster algebras for (quantum) coordinate rings of matrices and Grassmannians contain cluster variables of all degrees in $\mathbb{N}$. Next we consider the list (given by Felikson, Shapiro & Tumarkin) of mutation-finite quivers that do not correspond to triangulations of marked surfaces. We show that $X_7$ gives rise to only two degrees, both with infinitely many variables, and that $\widetilde{E}_6$, $\widetilde{E}_7$ and $\widetilde{E}_8$ give rise to infinitely many variables in some degrees. Finally, we study gradings arising from marked surfaces (see Fomin, Shapiro & Thurston). We adapt a definition by Muller to define the space of valuation functions on such a surface and prove combinatorially that it is isomorphic to the space of gradings on the associated cluster algebra. We illustrate this theory by applying it to the annulus with $n+m$ marked points. We show that the standard grading is of mixed type. We also give an alternative grading in which all degrees have infinitely many cluster variables.
math.RT math.AC math.CO
this thesis is concerned with studying the properties of gradings on several examples of cluster algebras primarily of infinite type we first consider two finite type cases b_n and c_n completing a classification by grabowski for coefficientfree finite type cluster algebras we then consider gradings arising from 3 times 3 skewsymmetric matrices we show that the mutationcyclic matrices give rise to gradings in which all degrees are positive and have only finitely many associated cluster variables excepting one particular case for the mutationacyclic matrices we prove that all occurring degrees have infinitely many variables we provide a sufficient condition for a graded cluster algebra generated by a quiver to have infinitely many degrees based on the presence of a subquiver in its mutation class we use this to show that the cluster algebras for quantum coordinate rings of matrices and grassmannians contain cluster variables of all degrees in mathbbn next we consider the list given by felikson shapiro tumarkin of mutationfinite quivers that do not correspond to triangulations of marked surfaces we show that x_7 gives rise to only two degrees both with infinitely many variables and that widetildee_6 widetildee_7 and widetildee_8 give rise to infinitely many variables in some degrees finally we study gradings arising from marked surfaces see fomin shapiro thurston we adapt a definition by muller to define the space of valuation functions on such a surface and prove combinatorially that it is isomorphic to the space of gradings on the associated cluster algebra we illustrate this theory by applying it to the annulus with nm marked points we show that the standard grading is of mixed type we also give an alternative grading in which all degrees have infinitely many cluster variables
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1,803.02342
Magic-angle graphene superlattices: a new platform for unconventional superconductivity
The understanding of strongly-correlated materials, and in particular unconventional superconductors, has puzzled physicists for decades. Such difficulties have stimulated new research paradigms, such as ultra-cold atom lattices for simulating quantum materials. Here we report on the realization of intrinsic unconventional superconductivity in a 2D superlattice created by stacking two graphene sheets with a small twist angle. For angles near $1.1^\circ$, the first `magic' angle, twisted bilayer graphene (TBG) exhibits ultra-flat bands near charge neutrality, which lead to correlated insulating states at half-filling. Upon electrostatic doping away from these correlated insulating states, we observe tunable zero-resistance states with a critical temperature $T_c$ up to 1.7 K. The temperature-density phase diagram shows similarities with that of the cuprates, including superconducting domes. Moreover, quantum oscillations indicate small Fermi surfaces near the correlated insulating phase, in analogy with under-doped cuprates. The relative high $T_c$, given such small Fermi surface (corresponding to a record-low 2D carrier density of $10^{11} \textrm{cm}^{-2}$ , renders TBG among the strongest coupling superconductors, in a regime close to the BCS-BEC crossover. These novel results establish TBG as the first purely carbon-based 2D superconductor and as a highly tunable platform to investigate strongly-correlated phenomena, which could lead to insights into the physics of high-$T_c$ superconductors and quantum spin liquids.
cond-mat.mes-hall cond-mat.str-el cond-mat.supr-con
the understanding of stronglycorrelated materials and in particular unconventional superconductors has puzzled physicists for decades such difficulties have stimulated new research paradigms such as ultracold atom lattices for simulating quantum materials here we report on the realization of intrinsic unconventional superconductivity in a 2d superlattice created by stacking two graphene sheets with a small twist angle for angles near 11circ the first magic angle twisted bilayer graphene tbg exhibits ultraflat bands near charge neutrality which lead to correlated insulating states at halffilling upon electrostatic doping away from these correlated insulating states we observe tunable zeroresistance states with a critical temperature t_c up to 17 k the temperaturedensity phase diagram shows similarities with that of the cuprates including superconducting domes moreover quantum oscillations indicate small fermi surfaces near the correlated insulating phase in analogy with underdoped cuprates the relative high t_c given such small fermi surface corresponding to a recordlow 2d carrier density of 1011 textrmcm2 renders tbg among the strongest coupling superconductors in a regime close to the bcsbec crossover these novel results establish tbg as the first purely carbonbased 2d superconductor and as a highly tunable platform to investigate stronglycorrelated phenomena which could lead to insights into the physics of hight_c superconductors and quantum spin liquids
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1,803.02343
Infinitely Many M2-instanton Corrections to M-theory on $G_2$-manifolds
We consider the non-perturbative superpotential for a class of four-dimensional $\mathcal N=1$ vacua obtained from M-theory on seven-manifolds with holonomy $G_2$. The class of $G_2$-holonomy manifolds we consider are so-called twisted connected sum (TCS) constructions, which have the topology of a K3-fibration over $S^3$. We show that the non-perturbative superpotential of M-theory on a class of TCS geometries receives infinitely many inequivalent M2-instanton contributions from infinitely many three-spheres, which we conjecture are supersymmetric (and thus associative) cycles. The rationale for our construction is provided by the duality chain of arXiv:1708.07215, which relates M-theory on TCS $G_2$-manifolds to $E_8\times E_8$ heterotic backgrounds on the Schoen Calabi-Yau threefold, as well as to F-theory on a K3-fibered Calabi-Yau fourfold. The latter are known to have an infinite number of instanton corrections to the superpotential and it is these contributions that we trace through the duality chain back to the $G_2$-compactification.
hep-th math.DG
we consider the nonperturbative superpotential for a class of fourdimensional mathcal n1 vacua obtained from mtheory on sevenmanifolds with holonomy g_2 the class of g_2holonomy manifolds we consider are socalled twisted connected sum tcs constructions which have the topology of a k3fibration over s3 we show that the nonperturbative superpotential of mtheory on a class of tcs geometries receives infinitely many inequivalent m2instanton contributions from infinitely many threespheres which we conjecture are supersymmetric and thus associative cycles the rationale for our construction is provided by the duality chain of arxiv170807215 which relates mtheory on tcs g_2manifolds to e_8times e_8 heterotic backgrounds on the schoen calabiyau threefold as well as to ftheory on a k3fibered calabiyau fourfold the latter are known to have an infinite number of instanton corrections to the superpotential and it is these contributions that we trace through the duality chain back to the g_2compactification
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1,803.02344
A new family of analytical anisotropic solutions by gravitational decoupling
This work is focused in the study of analytic anisotropic solutions to Einstein's field equations, describing spherically symmetric and static configurations by way of the gravitational decoupling through the method of Minimal Geometric Deformation (MGD). For this we apply MGD to Heintzmann's solution obtaining two new analytic and well behaved anisotropic solutions, in which all their parameters such as the effective density, the effective radial and tangential pressure, as well as radial and tangential sound speed, fulfill each of the requirements for the physical acceptability available in the literature.
gr-qc
this work is focused in the study of analytic anisotropic solutions to einsteins field equations describing spherically symmetric and static configurations by way of the gravitational decoupling through the method of minimal geometric deformation mgd for this we apply mgd to heintzmanns solution obtaining two new analytic and well behaved anisotropic solutions in which all their parameters such as the effective density the effective radial and tangential pressure as well as radial and tangential sound speed fulfill each of the requirements for the physical acceptability available in the literature
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1,803.02345
State diagram of a three-sphere microswimmer in a channel
Geometric confinements are frequently encountered in soft matter systems and in particular significantly alter the dynamics of swimming microorganisms in viscous media. Surface-related effects on the motility of microswimmers can lead to important consequences in a large number of biological systems, such as biofilm formation, bacterial adhesion and microbial activity. On the basis of low-Reynolds-number hydrodynamics, we explore the state diagram of a three-sphere microswimmer under channel confinement in a slit geometry and fully characterize the swimming behavior and trajectories for neutral swimmers, puller- and pusher-type swimmers. While pushers always end up trapped at the channel walls, neutral swimmers and pullers may further perform a gliding motion and maintain a stable navigation along the channel. We find that the resulting dynamical system exhibits a supercritical pitchfork bifurcation in which swimming in the mid-plane becomes unstable beyond a transition channel height while two new stable limit cycles or fixed points that are symmetrically disposed with respect to the channel mid-height emerge. Additionally, we show that an accurate description of the averaged swimming velocity and rotation rate in a channel can be captured analytically using the method of hydrodynamic images, provided that the swimmer size is much smaller than the channel height.
physics.flu-dyn physics.bio-ph
geometric confinements are frequently encountered in soft matter systems and in particular significantly alter the dynamics of swimming microorganisms in viscous media surfacerelated effects on the motility of microswimmers can lead to important consequences in a large number of biological systems such as biofilm formation bacterial adhesion and microbial activity on the basis of lowreynoldsnumber hydrodynamics we explore the state diagram of a threesphere microswimmer under channel confinement in a slit geometry and fully characterize the swimming behavior and trajectories for neutral swimmers puller and pushertype swimmers while pushers always end up trapped at the channel walls neutral swimmers and pullers may further perform a gliding motion and maintain a stable navigation along the channel we find that the resulting dynamical system exhibits a supercritical pitchfork bifurcation in which swimming in the midplane becomes unstable beyond a transition channel height while two new stable limit cycles or fixed points that are symmetrically disposed with respect to the channel midheight emerge additionally we show that an accurate description of the averaged swimming velocity and rotation rate in a channel can be captured analytically using the method of hydrodynamic images provided that the swimmer size is much smaller than the channel height
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1,803.02346
The structure and stability of orbits in Hoag-like ring systems
Ring galaxies are amazing objects exemplified by the famous case of the Hoag's Object. Here the mass of the central galaxy may be comparable to the mass of the ring, making it a difficult case to model mechanically. In a previous paper, it was shown that the outer potential of a torus (ring) can be represented with good accuracy by the potential of a massive circle with the same mass. This approach allows us to simplify the problem of the particle motion in the gravitational field of a torus associated with a central mass by replacing the torus with a massive circle. In such a system there is a circle of unstable equilibrium that we call "Lagrangian circle" (LC). Stable circular orbits exist only in some region limited by the last possible circular orbit related to the disappearance of the extrema of the effective potential. We call this orbit "the outermost stable circular orbit" (OSCO) by analogy with the innermost stable circular orbit (ISCO) in the relativistic case of a black hole. Under these conditions, there is a region between OSCO and LC where the circular motion is not possible due to the competition between the gravitational forces by the central mass and the ring. As a result, a gap in the matter distribution can form in Hoag-like system with massive rings.
astro-ph.GA
ring galaxies are amazing objects exemplified by the famous case of the hoags object here the mass of the central galaxy may be comparable to the mass of the ring making it a difficult case to model mechanically in a previous paper it was shown that the outer potential of a torus ring can be represented with good accuracy by the potential of a massive circle with the same mass this approach allows us to simplify the problem of the particle motion in the gravitational field of a torus associated with a central mass by replacing the torus with a massive circle in such a system there is a circle of unstable equilibrium that we call lagrangian circle lc stable circular orbits exist only in some region limited by the last possible circular orbit related to the disappearance of the extrema of the effective potential we call this orbit the outermost stable circular orbit osco by analogy with the innermost stable circular orbit isco in the relativistic case of a black hole under these conditions there is a region between osco and lc where the circular motion is not possible due to the competition between the gravitational forces by the central mass and the ring as a result a gap in the matter distribution can form in hoaglike system with massive rings
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1,803.02347
Two results in metric fixed point theory
We establish two fixed point theorems for certain mappings of contractive type. The first result is concerned with the case where such mappings take a nonempty, closed subset of a complete metric space $X$ into $X$, and the second with an application of the continuation method to the case where they satisfy the Leray-Schauder boundary condition in Banach spaces.
math.FA math.CA
we establish two fixed point theorems for certain mappings of contractive type the first result is concerned with the case where such mappings take a nonempty closed subset of a complete metric space x into x and the second with an application of the continuation method to the case where they satisfy the lerayschauder boundary condition in banach spaces
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1,803.02348
Smoothed Action Value Functions for Learning Gaussian Policies
State-action value functions (i.e., Q-values) are ubiquitous in reinforcement learning (RL), giving rise to popular algorithms such as SARSA and Q-learning. We propose a new notion of action value defined by a Gaussian smoothed version of the expected Q-value. We show that such smoothed Q-values still satisfy a Bellman equation, making them learnable from experience sampled from an environment. Moreover, the gradients of expected reward with respect to the mean and covariance of a parameterized Gaussian policy can be recovered from the gradient and Hessian of the smoothed Q-value function. Based on these relationships, we develop new algorithms for training a Gaussian policy directly from a learned smoothed Q-value approximator. The approach is additionally amenable to proximal optimization by augmenting the objective with a penalty on KL-divergence from a previous policy. We find that the ability to learn both a mean and covariance during training leads to significantly improved results on standard continuous control benchmarks.
cs.LG cs.AI
stateaction value functions ie qvalues are ubiquitous in reinforcement learning rl giving rise to popular algorithms such as sarsa and qlearning we propose a new notion of action value defined by a gaussian smoothed version of the expected qvalue we show that such smoothed qvalues still satisfy a bellman equation making them learnable from experience sampled from an environment moreover the gradients of expected reward with respect to the mean and covariance of a parameterized gaussian policy can be recovered from the gradient and hessian of the smoothed qvalue function based on these relationships we develop new algorithms for training a gaussian policy directly from a learned smoothed qvalue approximator the approach is additionally amenable to proximal optimization by augmenting the objective with a penalty on kldivergence from a previous policy we find that the ability to learn both a mean and covariance during training leads to significantly improved results on standard continuous control benchmarks
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1,803.02349
Billion-scale Commodity Embedding for E-commerce Recommendation in Alibaba
Recommender systems (RSs) have been the most important technology for increasing the business in Taobao, the largest online consumer-to-consumer (C2C) platform in China. The billion-scale data in Taobao creates three major challenges to Taobao's RS: scalability, sparsity and cold start. In this paper, we present our technical solutions to address these three challenges. The methods are based on the graph embedding framework. We first construct an item graph from users' behavior history. Each item is then represented as a vector using graph embedding. The item embeddings are employed to compute pairwise similarities between all items, which are then used in the recommendation process. To alleviate the sparsity and cold start problems, side information is incorporated into the embedding framework. We propose two aggregation methods to integrate the embeddings of items and the corresponding side information. Experimental results from offline experiments show that methods incorporating side information are superior to those that do not. Further, we describe the platform upon which the embedding methods are deployed and the workflow to process the billion-scale data in Taobao. Using online A/B test, we show that the online Click-Through-Rate (CTRs) are improved comparing to the previous recommendation methods widely used in Taobao, further demonstrating the effectiveness and feasibility of our proposed methods in Taobao's live production environment.
cs.IR cs.AI
recommender systems rss have been the most important technology for increasing the business in taobao the largest online consumertoconsumer c2c platform in china the billionscale data in taobao creates three major challenges to taobaos rs scalability sparsity and cold start in this paper we present our technical solutions to address these three challenges the methods are based on the graph embedding framework we first construct an item graph from users behavior history each item is then represented as a vector using graph embedding the item embeddings are employed to compute pairwise similarities between all items which are then used in the recommendation process to alleviate the sparsity and cold start problems side information is incorporated into the embedding framework we propose two aggregation methods to integrate the embeddings of items and the corresponding side information experimental results from offline experiments show that methods incorporating side information are superior to those that do not further we describe the platform upon which the embedding methods are deployed and the workflow to process the billionscale data in taobao using online ab test we show that the online clickthroughrate ctrs are improved comparing to the previous recommendation methods widely used in taobao further demonstrating the effectiveness and feasibility of our proposed methods in taobaos live production environment
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1,803.0235
Degeneracy of gravitational waveforms in the context of GW150914
We study the degeneracy of theoretical gravitational waveforms for binary black hole mergers using an aligned-spin effective-one-body model. After appropriate truncation, bandpassing, and matching, we identify regions in the mass--spin parameter space containing waveforms similar to the template proposed for GW150914, with masses $m_1 = 36^{+5}_{-4} M_\odot$ and $m_2 = 29^{+4}_{-4} M_\odot$, using the cross-correlation coefficient as a measure of the similarity between waveforms. Remarkably high cross-correlations are found across broad regions of parameter space. The associated uncertanties exceed these from LIGO's Bayesian analysis considerably. We have shown that waveforms with greatly increased masses, such as $m_1 = 70 M_\odot$ and $m_2 = 35 M_\odot$, and strong anti-aligned spins ($\chi_1=0.95$ and $\chi_2=-0.95$) yield almost the same signal-to-noise ratio in the strain data for GW150914.
gr-qc astro-ph.CO
we study the degeneracy of theoretical gravitational waveforms for binary black hole mergers using an alignedspin effectiveonebody model after appropriate truncation bandpassing and matching we identify regions in the massspin parameter space containing waveforms similar to the template proposed for gw150914 with masses m_1 365_4 m_odot and m_2 294_4 m_odot using the crosscorrelation coefficient as a measure of the similarity between waveforms remarkably high crosscorrelations are found across broad regions of parameter space the associated uncertanties exceed these from ligos bayesian analysis considerably we have shown that waveforms with greatly increased masses such as m_1 70 m_odot and m_2 35 m_odot and strong antialigned spins chi_1095 and chi_2095 yield almost the same signaltonoise ratio in the strain data for gw150914
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1,803.02351
Time-dependent Features in the Primordial Spectrum
In a Quantum Field Theory with a time-dependent background, time-translational symmetry is broken. We therefore expect time-dependent loop corrections to cosmological observables after renormalization for an interacting field, with the consequent physical implications. In this paper we compute and discuss such radiative corrections to the primordial spectrum within simple models, both for massless and massive virtual fields, and we disentangle the time-dependence caused by the background and by the initial state after renormalization. For the investigated models the departure from near-scale-invariance is very small and there is full compatibility with the current Planck data constraints. Future CMB measurements may improve the current constraints on feature-full primordial spectra and possibly observe these effects in the most optimistic scenario of hybrid inflation, revealing the interacting nature of the inflaton field.
gr-qc hep-ph hep-th
in a quantum field theory with a timedependent background timetranslational symmetry is broken we therefore expect timedependent loop corrections to cosmological observables after renormalization for an interacting field with the consequent physical implications in this paper we compute and discuss such radiative corrections to the primordial spectrum within simple models both for massless and massive virtual fields and we disentangle the timedependence caused by the background and by the initial state after renormalization for the investigated models the departure from nearscaleinvariance is very small and there is full compatibility with the current planck data constraints future cmb measurements may improve the current constraints on featurefull primordial spectra and possibly observe these effects in the most optimistic scenario of hybrid inflation revealing the interacting nature of the inflaton field
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1,803.02352
Genealogy tree: understanding academic lineage of authors via algorithmic and visual analysis
Ancestry and genealogy tree are proven tools to determine the lineage of any person and establish dependencies among individuals. Genealogy tree can be exploited further to gain information about the researcher and his scholastic lineage which is of paramount importance in today's world of computer technology. this insight into academic genealogy could be a way of helping PHD students achieve academic socialization within the discipline, by making explicit connections that may be influential. Awareness of his scientific heritage gives the user a broader perspective of his own research project. This paper also highlights and investigates how this academic network is exploited by certain researchers using various visualization tools. It was observed during this work that the credibility and influence factor is determined by the various citations obtained by an author and to improve their rankings in various forms, they tend to collaborate in their academic circle and boost their citation count. A recent trend among researchers is to form communities based on their academic relationships and rely on copious citations for their mutual benefit. Tracing the genealogical relationships can be helpful in detecting such communities and also create a more quality aware metric using a lineage independent model for computation of author level metrics.
cs.DL
ancestry and genealogy tree are proven tools to determine the lineage of any person and establish dependencies among individuals genealogy tree can be exploited further to gain information about the researcher and his scholastic lineage which is of paramount importance in todays world of computer technology this insight into academic genealogy could be a way of helping phd students achieve academic socialization within the discipline by making explicit connections that may be influential awareness of his scientific heritage gives the user a broader perspective of his own research project this paper also highlights and investigates how this academic network is exploited by certain researchers using various visualization tools it was observed during this work that the credibility and influence factor is determined by the various citations obtained by an author and to improve their rankings in various forms they tend to collaborate in their academic circle and boost their citation count a recent trend among researchers is to form communities based on their academic relationships and rely on copious citations for their mutual benefit tracing the genealogical relationships can be helpful in detecting such communities and also create a more quality aware metric using a lineage independent model for computation of author level metrics
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1,803.02353
Multi-level Attention Model for Weakly Supervised Audio Classification
In this paper, we propose a multi-level attention model to solve the weakly labelled audio classification problem. The objective of audio classification is to predict the presence or absence of audio events in an audio clip. Recently, Google published a large scale weakly labelled dataset called Audio Set, where each audio clip contains only the presence or absence of the audio events, without the onset and offset time of the audio events. Our multi-level attention model is an extension to the previously proposed single-level attention model. It consists of several attention modules applied on intermediate neural network layers. The output of these attention modules are concatenated to a vector followed by a multi-label classifier to make the final prediction of each class. Experiments shown that our model achieves a mean average precision (mAP) of 0.360, outperforms the state-of-the-art single-level attention model of 0.327 and Google baseline of 0.314.
eess.AS cs.SD
in this paper we propose a multilevel attention model to solve the weakly labelled audio classification problem the objective of audio classification is to predict the presence or absence of audio events in an audio clip recently google published a large scale weakly labelled dataset called audio set where each audio clip contains only the presence or absence of the audio events without the onset and offset time of the audio events our multilevel attention model is an extension to the previously proposed singlelevel attention model it consists of several attention modules applied on intermediate neural network layers the output of these attention modules are concatenated to a vector followed by a multilabel classifier to make the final prediction of each class experiments shown that our model achieves a mean average precision map of 0360 outperforms the stateoftheart singlelevel attention model of 0327 and google baseline of 0314
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1,803.02354
A Phase-Field Model for Fluid-Structure-Interaction
In this paper, we develop a novel phase-field model for fluid-structure interaction (FSI), that is capable to handle very large deformations as well as topology changes like contact of the solid to the domain boundary. The model is based on a fully Eulerian description of the velocity field in both, the fluid and the elastic domain. Viscous and elastic stresses in the Navier-Stokes equations are restricted to the corresponding domains by multiplication with their characteristic functions. To obtain the elastic stress, an additional Oldroyd-B - like equation is solved. Thermodynamically consistent forces are derived by energy variation. The convergence of the derived equations to the traditional sharp interface formulation of fluid-structure interaction is shown by matched asymptotic analysis. The model is evaluated in a challenging benchmark scenario of an elastic body traversing a fluid channel. A comparison to reference values from Arbitrary Lagrangian Eulerian (ALE) simulations shows very good agreement. We highlight some distinct advantages of the new model, like the avoidance of re-triangulations and the stable inclusion of surface tension. Further, we demonstrate how simple it is to include contact dynamics into the model, by simulating a ball bouncing off a wall. We extend this scenario to include adhesion of the ball, which to our knowledge, cannot be simulated with any other FSI model. While we have restricted simulations to fluid-structure interaction, the model is capable to simulate any combination of viscous fluids, visco-elastic fluids and elastic solids.
physics.comp-ph physics.flu-dyn
in this paper we develop a novel phasefield model for fluidstructure interaction fsi that is capable to handle very large deformations as well as topology changes like contact of the solid to the domain boundary the model is based on a fully eulerian description of the velocity field in both the fluid and the elastic domain viscous and elastic stresses in the navierstokes equations are restricted to the corresponding domains by multiplication with their characteristic functions to obtain the elastic stress an additional oldroydb like equation is solved thermodynamically consistent forces are derived by energy variation the convergence of the derived equations to the traditional sharp interface formulation of fluidstructure interaction is shown by matched asymptotic analysis the model is evaluated in a challenging benchmark scenario of an elastic body traversing a fluid channel a comparison to reference values from arbitrary lagrangian eulerian ale simulations shows very good agreement we highlight some distinct advantages of the new model like the avoidance of retriangulations and the stable inclusion of surface tension further we demonstrate how simple it is to include contact dynamics into the model by simulating a ball bouncing off a wall we extend this scenario to include adhesion of the ball which to our knowledge cannot be simulated with any other fsi model while we have restricted simulations to fluidstructure interaction the model is capable to simulate any combination of viscous fluids viscoelastic fluids and elastic solids
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1,803.02355
Cosmological bounds on the field content of asymptotically safe gravity-matter models
We use the non-Gaussian fixed points (NGFPs) appearing in the renormalization group flow of gravity and gravity-matter systems to construct models of NGFP-driven inflation via a renormalization group improvement scheme. The cosmological predictions of these models depend sensitively on the characteristic properties of the NGFPs, including their position and stability coefficients, which in turn are determined by the field content of the underlying matter sector. We demonstrate that the NGFPs appearing in gravity-matter systems where the matter content is close to the one of the standard model of particle physics are the ones compatible with cosmological data. Somewhat counterintuitively, the negative fixed point value of the dimensionless cosmological constant is essential for these findings.
gr-qc hep-th
we use the nongaussian fixed points ngfps appearing in the renormalization group flow of gravity and gravitymatter systems to construct models of ngfpdriven inflation via a renormalization group improvement scheme the cosmological predictions of these models depend sensitively on the characteristic properties of the ngfps including their position and stability coefficients which in turn are determined by the field content of the underlying matter sector we demonstrate that the ngfps appearing in gravitymatter systems where the matter content is close to the one of the standard model of particle physics are the ones compatible with cosmological data somewhat counterintuitively the negative fixed point value of the dimensionless cosmological constant is essential for these findings
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1,803.02356
Complexity Functionals and Complexity Growth Limits in Continuous MERA Circuits
Using the path integral associated to a cMERA tensor network, we provide an operational definition for the complexity of a cMERA circuit/state which is relevant to investigate the complexity of states in quantum field theory. In this framework, it is possible to explicitly establish the correspondence (Minimal) Complexity $=$ (Least) Action. Remarkably, it is also shown how the cMERA complexity action functional can be seen as the action of a Liouville field theory, thus establishing a connection with two dimensional quantum gravity. Concretely, the Liouville mode is identified with the variational parameter defining the cMERA circuit. The rate of complexity growth along the cMERA renormalization group flow is obtained and shown to saturate limits which are in close resemblance to the fundamental bounds to the speed of evolution in unitary quantum dynamics, known as quantum speed limits. We also show that the complexity of a cMERA circuit measured through these complexity functionals, can be cast in terms of the variationally-optimized amount of left-right entanglement created along the cMERA renormalization flow. Our results suggest that the patterns of entanglement in states of a QFT could determine their dual gravitational descriptions through a principle of least complexity.
hep-th cond-mat.str-el quant-ph
using the path integral associated to a cmera tensor network we provide an operational definition for the complexity of a cmera circuitstate which is relevant to investigate the complexity of states in quantum field theory in this framework it is possible to explicitly establish the correspondence minimal complexity least action remarkably it is also shown how the cmera complexity action functional can be seen as the action of a liouville field theory thus establishing a connection with two dimensional quantum gravity concretely the liouville mode is identified with the variational parameter defining the cmera circuit the rate of complexity growth along the cmera renormalization group flow is obtained and shown to saturate limits which are in close resemblance to the fundamental bounds to the speed of evolution in unitary quantum dynamics known as quantum speed limits we also show that the complexity of a cmera circuit measured through these complexity functionals can be cast in terms of the variationallyoptimized amount of leftright entanglement created along the cmera renormalization flow our results suggest that the patterns of entanglement in states of a qft could determine their dual gravitational descriptions through a principle of least complexity
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1,803.02357
Revolutionizing Our Understanding of AGN Feedback and its Importance to Galaxy Evolution in the Era of the Next Generation Very Large Array
Energetic feedback by Active Galactic Nuclei (AGNs) plays an important evolutionary role in the regulation of star formation (SF) on galactic scales. However, the effects of this feedback as a function of redshift and galaxy properties such as mass, environment and cold gas content remain poorly understood. The broad frequency coverage (1 to 116 GHz), high sensitivity (up to ten times higher than the Karl G. Jansky Very Large Array), and superb angular resolution (maximum baselines of at least a few hundred km) of the proposed next generation Very Large Array (ngVLA) are uniquely poised to revolutionize our understanding of AGNs and their role in galaxy evolution. Here, we provide an overview of the science related to AGN feedback that will be possible in the ngVLA era and present new continuum ngVLA imaging simulations of resolved radio jets spanning a wide range of intrinsic extents. We also consider key computational challenges and discuss exciting opportunities for multi-wavelength synergy with other next-generation instruments, such as the Square Kilometer Array and the James Webb Space Telescope. The unique combination of high-resolution, large collecting area, and wide frequency range will enable significant advancements in our understanding of the effects of jet-driven feedback on sub-galactic scales, particularly for sources with extents of a few pc to a few kpc such as young and/or lower-power radio AGNs, AGNs hosted by low-mass galaxies, radio jets that are interacting strongly with the interstellar medium of the host galaxy, and AGNs at high redshift.
astro-ph.GA
energetic feedback by active galactic nuclei agns plays an important evolutionary role in the regulation of star formation sf on galactic scales however the effects of this feedback as a function of redshift and galaxy properties such as mass environment and cold gas content remain poorly understood the broad frequency coverage 1 to 116 ghz high sensitivity up to ten times higher than the karl g jansky very large array and superb angular resolution maximum baselines of at least a few hundred km of the proposed next generation very large array ngvla are uniquely poised to revolutionize our understanding of agns and their role in galaxy evolution here we provide an overview of the science related to agn feedback that will be possible in the ngvla era and present new continuum ngvla imaging simulations of resolved radio jets spanning a wide range of intrinsic extents we also consider key computational challenges and discuss exciting opportunities for multiwavelength synergy with other nextgeneration instruments such as the square kilometer array and the james webb space telescope the unique combination of highresolution large collecting area and wide frequency range will enable significant advancements in our understanding of the effects of jetdriven feedback on subgalactic scales particularly for sources with extents of a few pc to a few kpc such as young andor lowerpower radio agns agns hosted by lowmass galaxies radio jets that are interacting strongly with the interstellar medium of the host galaxy and agns at high redshift
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1,803.02358
The 4:1 Outer Lindblad Resonance of a long slow bar as a potential explanation for the Hercules stream
There are multiple groups of comoving stars in the Solar neighbourhood, which can potentially be explained as the signatures of one of the fundamental resonances of non-axisymmetric structure such as the Galactic bar or spiral arms. One such stream, Hercules, has been proposed to result from the outer Lindblad resonance (OLR) of a short fast rotating bar as shown analytically, or the corotation resonance (CR) of a longer slower rotating bar as observed in an N-body model. We show that by including an m = 4 Fourier component in an analytical long bar model, with an amplitude that is typical for bars in N-body simulations, we can reproduce a Hercules like feature in the kinematics of the Solar neighbourhood. We then describe the expected symmetry in the velocity distribution arising from such a model, which we will soon be able to test with Gaia.
astro-ph.GA
there are multiple groups of comoving stars in the solar neighbourhood which can potentially be explained as the signatures of one of the fundamental resonances of nonaxisymmetric structure such as the galactic bar or spiral arms one such stream hercules has been proposed to result from the outer lindblad resonance olr of a short fast rotating bar as shown analytically or the corotation resonance cr of a longer slower rotating bar as observed in an nbody model we show that by including an m 4 fourier component in an analytical long bar model with an amplitude that is typical for bars in nbody simulations we can reproduce a hercules like feature in the kinematics of the solar neighbourhood we then describe the expected symmetry in the velocity distribution arising from such a model which we will soon be able to test with gaia
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1,803.02359
Dynamical structure factor of the $J_1-J_2$ Heisenberg model in one dimension: the variational Monte Carlo approach
The dynamical spin structure factor is computed within a variational framework to study the one-dimensional $J_1-J_2$ Heisenberg model. Starting from Gutzwiller-projected fermionic wave functions, the low-energy spectrum is constructed from two-spinon excitations. The direct comparison with Lanczos calculations on small clusters demonstrates the excellent description of both gapless and gapped (dimerized) phases, also including incommensurate structures for $J_2/J_1>0.5$. Calculations on large clusters show how the intensity evolves when increasing the frustrating ratio and give an unprecedented accurate characterization of the dynamical properties of (non-integrable) frustrated spin models.
cond-mat.str-el
the dynamical spin structure factor is computed within a variational framework to study the onedimensional j_1j_2 heisenberg model starting from gutzwillerprojected fermionic wave functions the lowenergy spectrum is constructed from twospinon excitations the direct comparison with lanczos calculations on small clusters demonstrates the excellent description of both gapless and gapped dimerized phases also including incommensurate structures for j_2j_105 calculations on large clusters show how the intensity evolves when increasing the frustrating ratio and give an unprecedented accurate characterization of the dynamical properties of nonintegrable frustrated spin models
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1,803.0236
Gaussian optimizers for entropic inequalities in quantum information
We survey the state of the art for the proof of the quantum Gaussian optimizer conjectures of quantum information theory. These fundamental conjectures state that quantum Gaussian input states are the solution to several optimization problems involving quantum Gaussian channels. These problems are the quantum counterpart of three fundamental results of functional analysis and probability: the Entropy Power Inequality, the sharp Young's inequality for convolutions, and the theorem "Gaussian kernels have only Gaussian maximizers." Quantum Gaussian channels play a key role in quantum communication theory: they are the quantum counterpart of Gaussian integral kernels and provide the mathematical model for the propagation of electromagnetic waves in the quantum regime. The quantum Gaussian optimizer conjectures are needed to determine the maximum communication rates over optical fibers and free space. The restriction of the quantum-limited Gaussian attenuator to input states diagonal in the Fock basis coincides with the thinning, which is the analog of the rescaling for positive integer random variables. Quantum Gaussian channels provide then a bridge between functional analysis and discrete probability.
math-ph cs.IT math.FA math.IT math.MP math.PR quant-ph
we survey the state of the art for the proof of the quantum gaussian optimizer conjectures of quantum information theory these fundamental conjectures state that quantum gaussian input states are the solution to several optimization problems involving quantum gaussian channels these problems are the quantum counterpart of three fundamental results of functional analysis and probability the entropy power inequality the sharp youngs inequality for convolutions and the theorem gaussian kernels have only gaussian maximizers quantum gaussian channels play a key role in quantum communication theory they are the quantum counterpart of gaussian integral kernels and provide the mathematical model for the propagation of electromagnetic waves in the quantum regime the quantum gaussian optimizer conjectures are needed to determine the maximum communication rates over optical fibers and free space the restriction of the quantumlimited gaussian attenuator to input states diagonal in the fock basis coincides with the thinning which is the analog of the rescaling for positive integer random variables quantum gaussian channels provide then a bridge between functional analysis and discrete probability
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1,803.02361
Galaxy clusters in simulations of the local Universe: a matter of constraints
To study the full formation and evolution history of galaxy clusters and their population, high resolution simulations of the latter are flourishing. However comparing observed clusters to the simulated ones on a one-to-one basis to refine the models and theories down to the details is non trivial. The large variety of clusters limits the comparisons between observed and numerical clusters. Simulations resembling the local Universe down to the cluster scales permit pushing the limit. Simulated and observed clusters can be matched on a one-to-one basis for direct comparisons provided that clusters are well reproduced besides being in the proper large scale environment. Comparing random and local-Universe like simulations obtained with differently grouped observational catalogs of peculiar velocities, this paper shows that the grouping scheme used to remove non-linear motions in the catalogs that constrain the simulations affects the quality of the numerical clusters. With a less aggressive grouping scheme - galaxies still falling onto clusters are preserved - combined with a bias minimization scheme, the mass of the dark matter halos, simulacra for 5 local clusters - Virgo, Centaurus, Coma, Hydra and Perseus - is increased by 39% closing the gap with observational mass estimates. Simulacra are found on average in 89% of the simulations, an increase of 5% with respect to the previous grouping scheme. The only exception is Perseus. Since the Perseus-Pisces region is not well covered by the used peculiar velocity catalog, the latest release let us foresee a better simulacrum for Perseus in a near future.
astro-ph.CO
to study the full formation and evolution history of galaxy clusters and their population high resolution simulations of the latter are flourishing however comparing observed clusters to the simulated ones on a onetoone basis to refine the models and theories down to the details is non trivial the large variety of clusters limits the comparisons between observed and numerical clusters simulations resembling the local universe down to the cluster scales permit pushing the limit simulated and observed clusters can be matched on a onetoone basis for direct comparisons provided that clusters are well reproduced besides being in the proper large scale environment comparing random and localuniverse like simulations obtained with differently grouped observational catalogs of peculiar velocities this paper shows that the grouping scheme used to remove nonlinear motions in the catalogs that constrain the simulations affects the quality of the numerical clusters with a less aggressive grouping scheme galaxies still falling onto clusters are preserved combined with a bias minimization scheme the mass of the dark matter halos simulacra for 5 local clusters virgo centaurus coma hydra and perseus is increased by 39 closing the gap with observational mass estimates simulacra are found on average in 89 of the simulations an increase of 5 with respect to the previous grouping scheme the only exception is perseus since the perseuspisces region is not well covered by the used peculiar velocity catalog the latest release let us foresee a better simulacrum for perseus in a near future
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1,803.02362
IceCube bounds on sterile neutrinos above 10 eV
We study the capabilities of IceCube to search for sterile neutrinos with masses above 10 eV by analyzing its $\nu_\mu$ disappearance atmospheric neutrino sample. We find that IceCube is not only sensitive to the mixing of sterile neutrinos to muon neutrinos, but also to the more elusive mixing with tau neutrinos through matter effects. The currently released 1-year data shows a mild (around 2$\sigma$) preference for non-zero sterile mixing, which overlaps with the favoured region for the sterile neutrino interpretation of the ANITA upward shower. Although the null results from CHORUS and NOMAD on $\nu_\mu$ to $\nu_\tau$ oscillations in vacuum disfavour the hint from the IceCube 1-year data, the relevant oscillation channel and underlying physics are different. At the $99\%$ C.L. an upper bound is obtained instead that improves over the present Super-Kamiokande and DeepCore constraints in some parts of the parameter space. We also investigate the physics reach of the roughly 8 years of data that is already on tape as well as a forecast of 20 years data to probe the present hint or improve upon current constraints.
hep-ph
we study the capabilities of icecube to search for sterile neutrinos with masses above 10 ev by analyzing its nu_mu disappearance atmospheric neutrino sample we find that icecube is not only sensitive to the mixing of sterile neutrinos to muon neutrinos but also to the more elusive mixing with tau neutrinos through matter effects the currently released 1year data shows a mild around 2sigma preference for nonzero sterile mixing which overlaps with the favoured region for the sterile neutrino interpretation of the anita upward shower although the null results from chorus and nomad on nu_mu to nu_tau oscillations in vacuum disfavour the hint from the icecube 1year data the relevant oscillation channel and underlying physics are different at the 99 cl an upper bound is obtained instead that improves over the present superkamiokande and deepcore constraints in some parts of the parameter space we also investigate the physics reach of the roughly 8 years of data that is already on tape as well as a forecast of 20 years data to probe the present hint or improve upon current constraints
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1,803.02363
Merger history of central galaxies in Semi-Analytic Models of galaxy formation
We investigate the dynamical evolution of galaxies in groups with different formation epochs. Galaxy groups have been selected to be in different dynamical states, namely dynamically old and dynamically young, which reflect their early and late formation times, respectively, based on their halo mass assembly. Brightest galaxies in dynamically young groups have suffered their last major galaxy merger typically $\sim 2$ Gyr more recently than their counterparts in dynamically old groups. Furthermore, we study the evolution of velocity dispersion in these two classes and compare them with the analytic models of isolated halos. The velocity dispersion of dwarf galaxies in high mass, dynamically young groups increases slowly in time, while the analogous dispersion in dynamically old high-mass groups is constant. In contrast, the velocity dispersion of giant galaxies in low mass groups decreases rapidly at late times. This increasing velocity bias is caused by dynamical friction, and starts much earlier in the dynamically old groups. The recent {\sc Radio-SAGE} model of galaxy formation suggests that radio luminosities of central galaxies, considered to be tracers of AGN activity, are enhanced in halos that assembled more recently, independent of the time since the last major merger.
astro-ph.GA
we investigate the dynamical evolution of galaxies in groups with different formation epochs galaxy groups have been selected to be in different dynamical states namely dynamically old and dynamically young which reflect their early and late formation times respectively based on their halo mass assembly brightest galaxies in dynamically young groups have suffered their last major galaxy merger typically sim 2 gyr more recently than their counterparts in dynamically old groups furthermore we study the evolution of velocity dispersion in these two classes and compare them with the analytic models of isolated halos the velocity dispersion of dwarf galaxies in high mass dynamically young groups increases slowly in time while the analogous dispersion in dynamically old highmass groups is constant in contrast the velocity dispersion of giant galaxies in low mass groups decreases rapidly at late times this increasing velocity bias is caused by dynamical friction and starts much earlier in the dynamically old groups the recent sc radiosage model of galaxy formation suggests that radio luminosities of central galaxies considered to be tracers of agn activity are enhanced in halos that assembled more recently independent of the time since the last major merger
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1,803.02364
On the behaviour of composite resonances breaking lepton flavour universality
Within the context of composite Higgs models, recent hints on lepton-flavour non-universality in $B$ decays can be explained by a vector resonance $V$ with sizeable couplings to the Standard Model leptons ($\ell$). We argue that, in such a case, spin-$1/2$ leptonic resonances ($L$) are most probably light enough to open the decay mode $V \rightarrow L\ell$. This implies, in combination with the fact that couplings between composite resonances are much larger than those between composite and elementary fields, that this new decay can be important. In this paper, we explore under which conditions it dominates over other decay modes. Its discovery, however, requires a dedicated search strategy. Employing jet substructure techniques, we analyse the final state with largest branching ratio, namely $\mu^+\mu^- Z/h, Z/h \rightarrow$ jets. We show that (i) parameter space regions that were believed excluded by di-muon searches are still allowed, (ii) these regions can already be tested with the dedicated search we propose and (iii) $V$ masses as large as $\sim 3.5$ TeV can be probed at the LHC during the high-luminosity phase.
hep-ph
within the context of composite higgs models recent hints on leptonflavour nonuniversality in b decays can be explained by a vector resonance v with sizeable couplings to the standard model leptons ell we argue that in such a case spin12 leptonic resonances l are most probably light enough to open the decay mode v rightarrow lell this implies in combination with the fact that couplings between composite resonances are much larger than those between composite and elementary fields that this new decay can be important in this paper we explore under which conditions it dominates over other decay modes its discovery however requires a dedicated search strategy employing jet substructure techniques we analyse the final state with largest branching ratio namely mumu zh zh rightarrow jets we show that i parameter space regions that were believed excluded by dimuon searches are still allowed ii these regions can already be tested with the dedicated search we propose and iii v masses as large as sim 35 tev can be probed at the lhc during the highluminosity phase
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1,803.02365
Strong Hydrogen Absorption at Cosmic Dawn: the Signature of a Baryonic Universe
The recently reported detection of redshifted 21cm absorption at $z \approx 17$ is a significant advance in the exploration of the cosmic dark ages. The observed signal ($T_{\mathrm{21}} \approx -0.5$ K with the limit $T_{\mathrm{21}} < -0.3$ K at 99\% c.l.) is anomalously strong for $\Lambda$CDM, which predicts at most $-0.24$ K. Here I show that the strong observed signal is expected in a purely baryonic universe.
astro-ph.CO
the recently reported detection of redshifted 21cm absorption at z approx 17 is a significant advance in the exploration of the cosmic dark ages the observed signal t_mathrm21 approx 05 k with the limit t_mathrm21 03 k at 99 cl is anomalously strong for lambdacdm which predicts at most 024 k here i show that the strong observed signal is expected in a purely baryonic universe
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1,803.02366
Dynamic suppression of Rayleigh light scattering in dielectric resonators
The ultimate limits of performance for any classical optical system are set by sub-wavelength fluctuations within the host material, that may be frozen-in or even dynamically induced. The most common manifestation of such sub-wavelength disorder is Rayleigh light scattering, which is observed in nearly all wave-guiding technologies today and can lead to both irreversible radiative losses as well as undesirable intermodal coupling. While it has been shown that backscattering from disorder can be suppressed by breaking time-reversal symmetry in magneto-optic and topological insulator materials, common optical dielectrics possess neither of these properties. Here we demonstrate an optomechanical approach for dynamically suppressing Rayleigh backscattering within dielectric resonators. We achieve this by locally breaking time-reversal symmetry in a silica resonator through a Brillouin scattering interaction that is available in all materials. Near-complete suppression of Rayleigh backscattering is experimentally confirmed through three independent measurements -- the reduction of the back-reflections caused by scatterers, the elimination of a commonly seen normal-mode splitting effect, and by measurement of the reduction in intrinsic optical loss. More broadly, our results provide new evidence that it is possible to dynamically suppress Rayleigh backscattering within any optical dielectric medium, for achieving robust light propagation in nanophotonic devices in spite of the presence of scatterers or defects.
physics.optics
the ultimate limits of performance for any classical optical system are set by subwavelength fluctuations within the host material that may be frozenin or even dynamically induced the most common manifestation of such subwavelength disorder is rayleigh light scattering which is observed in nearly all waveguiding technologies today and can lead to both irreversible radiative losses as well as undesirable intermodal coupling while it has been shown that backscattering from disorder can be suppressed by breaking timereversal symmetry in magnetooptic and topological insulator materials common optical dielectrics possess neither of these properties here we demonstrate an optomechanical approach for dynamically suppressing rayleigh backscattering within dielectric resonators we achieve this by locally breaking timereversal symmetry in a silica resonator through a brillouin scattering interaction that is available in all materials nearcomplete suppression of rayleigh backscattering is experimentally confirmed through three independent measurements the reduction of the backreflections caused by scatterers the elimination of a commonly seen normalmode splitting effect and by measurement of the reduction in intrinsic optical loss more broadly our results provide new evidence that it is possible to dynamically suppress rayleigh backscattering within any optical dielectric medium for achieving robust light propagation in nanophotonic devices in spite of the presence of scatterers or defects
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